Table 1: Overview of the observed sample.
Ident RA (2000) Dec RSA RC3 PA B0 (B-V)0 (U-B)0 $V_{\rm hel}$ $r_{\rm e}$ $\rho_{xyz}$ $\epsilon$
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
Notes: the value of $r_{\rm e}$ of NGC 4696, NGC 5090 and NGC 5266 have been derived from ESO-LV
(Lauberts & Valentijn 1989) while the value for NGC 5044 is derived from Goudfrooij (1994).

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