\begin{table}%t1
\caption{Overview of the observed sample.}
%\centerline
{
\begin{tabular}{lcrllrrcrrclc}
 \hline\hline
\multicolumn{1}{c}{Ident}
& \multicolumn{2}{c}{RA (2000) Dec}
& \multicolumn{1}{c}{RSA}
& \multicolumn{1}{c}{RC3}
& \multicolumn{1}{c}{PA}
& \multicolumn{1}{c}{$B_0$}
& \multicolumn{1}{c}{$(B-V)_0$}
 & \multicolumn{1}{c}{$(U-B)_0$}
& \multicolumn{1}{c}{$V_{\rm hel}$}
& \multicolumn{1}{c}{$r_{\rm e}$}
& \multicolumn{1}{c}{$\rho_{xyz}$} 
& \multicolumn{1}{c}{$\epsilon$} \\
\hline
 NGC~3607 & 11 16 54.3 &  18 03 10 & S03(3)     & SA(s)0:       & 120 & 11.08 & 0.88 & 0.43 &  934 &  43.4  & 0.34 & 0.11 \\
 NGC~3818 & 11 41 57.3 &--06 09 20 &    E5        & E5              & 103 & 12.47 & 0.91 &         &1701 &  22.2  & 0.20 & 0.36 \\
 NGC~4374 & 12 25 03.7 &  12 53 13 &    E1        & E1              & 135 & 10.01 & 0.94 & 0.50 &1060 &  50.9  & 3.99 & 0.11\\
 NGC~4696 & 12 48 49.3 &--41 18 40 &    (E3)       & E+1 pec     &   95 & 10.85 &         &         &2958 &   85.0 & 0.00 & 0.34\\
 NGC~4697 & 12 48 35.9 &--05 48 03 &     E6       & E6              &   70 & 10.07 & 0.89 & 0.39 &1241 &  72.0  & 0.60 & 0.32\\
 NGC~5011 & 13 12 51.8 &--43 05 46 &     E2      & E1-2          & 154 & 11.90 & 0.89 &         &3104 &   23.8 & 0.27 & 0.15\\
 NGC~5044 & 13 15 24.0 &--16 23 08 &     E0      & E0              &   11 & 11.67 &         &         &2704 &  82.3  & 0.38 & 0.11\\
 NGC~5077 & 13 19 31.6 &--12 39 26 & S01/2(4)  & E3+           &  11 & 12.52 & 0.98 & 0.54 & 2764 & 22.8   & 0.23 & 0.15\\
 NGC~5090 & 13 21 12.8 &--43 42 16 &     E2      & E2              & 136& 11.97 &         &         & 3421 & 62.4   &         & 0.15\\
 NGC~5193 & 13 31 53.5 &--33 14 04 &    S01(0)  & E pec          &  71 & 12.35 & 0.86 &         & 3711 & 26.7   &         & 0.07\\
 & & & & & & & & & &  & &\\ 
 NGC~5266 & 13 43 02.1 &--48 10 10 &S03(5) pec&SA0-:          & 109& 11.50 &         &         & 3074 & 76.7   & 0.35 & 0.31\\
 NGC~5638 & 14 29 40.4 &  03 14 00 &   E1       &E1               &150 & 12.06 & 0.91 & 0.46 & 1676 & 28.0  &  0.79 & 0.11\\
 NGC~5812 & 15 00 55.7 &--07 27 26 &    E0        & E0              &130 & 11.83 & 0.94 &         & 1930 & 25.5  &  0.19 & 0.13\\
 NGC~5813 & 15 01 11.2 & 01 42 07  &   E1        &  E1-2         &145 & 11.42 & 0.94 & 0.52 & 1972 & 57.2  &  0.88 & 0.28\\
 NGC~5831 & 15 04 07.0 & 01 13 12  &   E4        & E3              &  55 & 12.31 & 0.92 & 0.55 & 1656 & 25.5  &  0.83 & 0.13\\
 NGC~5898 & 15 18 13.6 & --24 05 51& S02/3(0)  & E0             &  30  & 12.41 & 0.95 &         & 2267 & 22.2  & 0.23  & 0.07\\
 NGC~6758 & 19 13 52.3 & --56 18 36& E2 (merger) &  E+:           &  121& 12.31 & 0.96 & 0.44 & 3404 & 20.3  &          & 0.22\\
 NGC~6776 & 19 25 19.1 &--63 51 37 & E1 pec &  E+ pec      &   15 &  12.71& 0.86& 0.44  & 5480 & 17.7  &         &  0.17\\
\hline
\end{tabular}}
\label{table1}
\smallskip
 Notes: the value of $r_{\rm e}$ of NGC~4696, NGC~5090 and NGC~5266 have been derived from ESO-LV (Lauberts \& Valentijn  \cite{LV89})
while the value for NGC~5044 is derived from Goudfrooij (\cite{Gou94}). 
\end{table}