  Models of galaxy formation ultimately aim at reproducing the _observed_
properties of galaxies. We report on work in progress to predict luminosities,
colours and morphologies of field objects of various masses through N-body +
Smoothed Particle Hydrodynamics simulations. We describe our method, illustrate
the effects of varying the star formation assumptions, show some preliminary
results, draw encouragement from their strengths as well as lessons about what
improvements are most needed.
