filters for NGC 3808. Photometric calibration was accomplished using repeated observations of the $BVRI$ standard stars from Landolt (1983) and Smith et al. (1991). The seeing during our observations was about 2$\arcsec$. A log of observations is given in Table 1 (extinction corrected sky brightnesses in each frame in $\rm mag\,arcsec^{-2}$ are presented in the last column of the table). Reduction of the raw CCD data was made in standard manner (for details see Paper I - Reshetnikov et al. 1994). The ESO-MIDAS package (MIDAS User Guide 1994) was used.

[llllll]{}\
\
\
Object&Data&Band-& Exp. & Air- & Sky\
& &pass & (sec)& mass & mag.\
\
\
NGC 3808 & 10/11.03.94 & $V$ & 600 & 1.075 & 21.14\
& & $R$ & 300 & 1.079 & 20.66\
& & $I$ & 600 & 1.075 & 19.24\
\
NGC 6286 & 6/7.05.92 & $B$ & 1000& 1.049 & 21.94\
& & $V$ & 600 & 1.043 & 21.19\
& & $R$ & 300 & 1.040 & 20.58\
\

Spectral observations of the galaxies were obtained earlier at the 1.93-m telescope of the Observatoire de Haute-Provence, using the spectrograph CARELEC and the CCD TK512. For details of observations and reductions 