\begin{table}%t1
\caption{\label{tbgalfit}Properties of the target \object{J033210.76--274234.6}.}
\par
%\begin{center}
\par
\begin{tabular}{ccccccc}
\hline \hline
\multicolumn{4}{l}{\bf {\small Photometric properties:}} \\
  $M_B$(AB) &  $M_J$(AB) &   $R_{\rm half}$$^{*}$ & $M_{\rm stellar}^{\rm total}$ & {\it SFR}$_{\rm IR}$ & {\it SFR}$_{\rm 2800}$ & $A_V$ \\ 
            &            & (kpc) & ($10^{10}~M_\odot$)  &     ($M_\odot$/yr) &   ($M_\odot$/yr) & \\
   $-$21.78 & $-$23.70   & 4.36 &$27.5 $ & 5.27  & 3.24 & 0.2 \\ 
   \hline
\end{tabular}
\begin{tabular}{ccccc}
\multicolumn{5}{l}{\bf Morphological decomposition for $z$-band}  \\ 
& Magnitude & $R_{\rm eff}$$^{a}$~(kpc)&  $F_{i}$$^{b}$ & ~~~$B-z$$^{c}$ \\  \hline 
\multicolumn{1}{l|}{core-A} & 20.03 $\pm$ 0.01  &  1.78 $\pm$ 0.02& 0.27 $\pm$ 0.01 & ~~~3.53 \\
\multicolumn{1}{l|}{core-B}& 20.85 $\pm$ 0.01  &  0.74 $\pm$ 0.01& 0.13 $\pm$ 0.01 & ~~~3.15  \\
\multicolumn{1}{l|}{Disk \hphantom{Ring}}     & 19.14 $\pm$ 0.01&  5.39 $\pm$ 0.01& 0.60 $\pm$ 0.01 & ~~~2.94
\\ \hline 
\end{tabular}
\\
\begin{tabular}{ccccc}
& Center$^{d}$ & PA$^{e}$&  Inc.~(b~/~a)$^{f}$ & ~$M_{\rm stellar}$$^{g}$  \\
\multicolumn{1}{l}{} & (kpc) & ($^\circ$)   &  &  ($10^{10}~M_\odot$)   \\ \hline 
\multicolumn{1}{l|}{core-A} &  [0.00,   0.00] &~~~69  & 0.75   & ~~~~3.57   \\
\multicolumn{1}{l|}{core-B} &  [2.15, $-$0.10]     &~~~65  & 0.82   & ~~~~7.43   \\
\multicolumn{1}{l|}{Disk}     &[0.67,   0.03]     &~~~65  & 26$^\circ$   & 16.5   \\
\multicolumn{1}{l|}{Blue Ring}&[0.02,   0.12]  &$-$78 & 52$^\circ$ & --- \\ \hline 
\end{tabular}
\\
\begin{tabular}{ccccc}
\multicolumn{5}{l}{\bf Physical scales} \\
\multicolumn{2}{l}{The distance of the two cores} & 2.15 kpc &~~~~~~~~~~~~ &~~~~~~~~~~~~ \\
\multicolumn{2}{l}{The radius of the blue ring} & 7.18 kpc \\
\hline 
\end{tabular}
%\end{center}
\par
%\vglue 1mm
$^{*}$~The half-light radius;
$^{a}$~the effective radius of the S\'{e}rsic profile;
$^{b}$~the light fraction of each model component with respect to the total model flux;
$^{c}$~the $B-z$~color of each component, calculated based on the morphological decomposition;
$^{d}$~the center of each component, measured with respect to the center of the disk;
$^{e}$~the position angle of each component;
$^{f}$~for the disk and the ring we give the inclination in degrees; for the bulges we give the axis ratios;
$^{g}$~the stellar mass of each component (see Sect.~\ref{secmodel} for details).
\end{table}