  We present here a new set of evolutionary population synthesis models for
template galaxies along the Hubble morphological sequence. The models, that
account for the individual evolution of the bulge, disk, and halo components,
provide basic morphological features, along with bolometric luminosity and
color evolution (including Johnson/Cousins "UBVRcIcJHK", Gunn "gri", and
Washington "CMT1T2" photometric systems) between 1 and 15 Gyr. Luminosity
contribution from residual gas is also evaluated, both in terms of nebular
continuum and Balmer-line enhancement.
