Using a two-dimensional galaxy image decomposition technique, we extract gl
obal bulge and disk parameters for a complete sample of early-type disk gal
axies in the near-infrared K band. We find significant correlation of the b
ulge parameter n with the central bulge surface brightness mu(b)(0) and wit
h effective radius r(e). Using bivariate analysis techniques, we find that
log n, log r(e), and mu(b)(0) are distributed in a plane with small scatter
. We do not find a strong correlation of n with bulge-to-disk luminosity ra
tio, contrary to earlier reports. For these early-type disk galaxies, r(e)
and the disk scale length r(d) are well correlated, but with large scatter.
We examine the implications of our results for various bulge formation sce
narios in disk galaxies.