  We present R-band CCD photometry for 1332 early-type galaxies, observed as
part of the ENEAR survey of peculiar motions using early-type galaxies in the
nearby Universe. Circular apertures are used to trace the surface brightness
profiles, which are then fit by a two-component bulge-disk model. From the fits
we obtain the structural parameters required to estimate galaxy distances using
the D_n-sigma and Fundamental Plane relations. We find that about 12% of the
galaxies are well represented by a pure r^{1/4} law while 87% are best fit by a
two component model. There are 356 repeated observations of 257 galaxies
obtained during different runs that are used to derive statistical corrections
and bring the data to a common system. We also use these repeated observations
to estimate our internal errors. The accuracy of our measurements are tested by
the comparison of 354 galaxies in common with other authors. Typical errors in
our measurements are 0.011 dex for log{D_n}, 0.064 dex for log{r_e}, 0.086 mag
arcsec^{-2} for <{mu_e}> and 0.09 for m_{R_C}, comparable to those estimated by
other authors. The photometric data reported here represent one of the largest
high-quality and uniform all-sky samples currently available for early-type
galaxies in the nearby universe, especially suitable for peculiar motion
studies.
