  We propose a two dimensional galaxy fitting algorithm to extract parameters
of the bulge, disk, and a central point source from broad band images of
galaxies. We use a set of realistic galaxy parameters to construct a large
number of model galaxy images which we then use as input to our galaxy fitting
program to test it. We find that our approach recovers all structural
parameters to a fair degree of accuracy. We elucidate our procedures by
extracting parameters for 3 real galaxies -- NGC 661, NGC 1381, and NGC 1427.
