  We present one of the largest homogeneous sets of spiral and lenticular
galaxy brightness profile decompositions completed to date. The 659 galaxies in
our sample have been fitted with a deVaucouleurs' law for the bulge component
and an inner-truncated exponential for the disk component. Of the 659 galaxies
in the sample, 620 were successfully fit with the chosen fitting functions. The
fits are generally well-defined, with more than 90% having RMS deviations from
the observed profile of less than 0.35 magnitudes. We find no correlations of
fitting quality, as measured by these RMS residuals, with either morphological
type or inclination. Similarly, the estimated errors of the fitted coefficients
show no significant trends with type or inclination. These decompositions form
a useful basis for the study of the light distributions of spiral and
lenticular galaxies. The object base is sufficiently large that well-defined
samples of galaxies can be selected from it.
