  We have analyzed CCD images of 14 Abell clusters in the R filter of the SARS
survey (Way et al 2004), with cz<40000kms^{-1}. We have obtained the luminosity
profiles for 507 galaxies of which 232 (46%) have known redshifts. In order to
fit the luminosity profiles we used the de Vaucouleurs law for bulge systems,
an exponential profile for disk systems and we have also fitted the Sersic's
law (r^n) to all galaxy profiles. We have found that 162 (32%) galaxies in the
sample have pure r^{1/4} profiles, 168 (33%) have pure exponential profiles,
while 93 (18%) galaxies have luminosity profiles that are well fitted by a
combination of both bulge and disk profiles. On the other hand, we could not
fit the classical bulge + disk profile to the remaining 84 (17%) galaxies of
the sample. For such cases we have only used the Sersic law. We have also
analyzed how seeing and sky cleaning affect the structural and photometric
parameters obtained through profile fitting. In addition, we have studied
several relations between these parameters. We have found that bulges and disks
show consistency with a unique relation in the \mu_e - log(r_e) plane. We also
found that bulges and disks obey a magnitude-size relation in the sense that
large bulges and disks (large r_e values) have high luminosities. On the other
hand, Sersic law fitting parameters n, $rs$ and \mu_s show a strong correlation
in agreement with other authors suggesting the idea that not only ellipticals
but all galaxies are likely to be understood as a one parameter family.
