\begin{table}
\caption{NGC~6340 $r$-band light profile decomposition using the
three-component model.}
%\centerline
{\begin{tabular}{lccc}
\hline
\hline
& S\'ersic & 1st disc & 2nd disc \\
\hline
$r_e$~kpc & $0.195\pm0.003$ & & \\
$n$  & $1.66\pm0.04$ & & \\
$\mu_e$~mag~arcsec$^{-2}$ & $17.99\pm0.16$ & & \\
$\mu_{0}$~mag~arcsec$^{-2}$ & & $18.46\pm0.55$ & $19.60\pm0.15$ \\
$d_{{\rm exp}}$~kpc & & $0.49\pm0.02$ & $2.02\pm0.02$ \\
$\langle\mu\rangle_e$~mag~arcsec$^{-2}$ & $17.04\pm0.16$ & $19.59\pm0.55$ & $20.72\pm0.15$ \\
$M_{B}$~mag & $-16.88$ & $-17.47$ & $-19.41$ \\
\hline
\end{tabular}}
\par
All values are corrected for Galactic extinction. Absolute
magnitudes of the components are converted into the $B$-band
using the transformation\\ from \citet{FSI95} for lenticular
galaxies $B - r = 1.17$~mag. \label{tabdecomp}
\par
\end{table}