A substantial population of high-redshift, early-type galaxies is detected
in very deep UBVRIJHK images. Four elliptical profile galaxies are identifi
ed in the redshift range 1 < z < 2, with very red spectral energy distribut
ions implying ages of greater than or similar to 2 Gyr for standard passive
evolution. We also find later type IR-luminous galaxies at similarly high
redshift (10 objects with z > 1, H < 25), with weak UV emission implying si
ngle-burst ages of greater than or similar to 1 Gyr. The number and luminos
ity densities of these galaxies are comparable to the local E/S0-Sbc popula
tions for Omega(m) > 0.2, suggesting that the major fraction of luminous Hu
bble sequence galaxies has evolved little since z similar to 2. A highly co
mplete photometric redshift distribution is constructed to H = 25 (69 galax
ies) that shows a broad spread of redshift, peaking at z similar to 1.5, in
reasonable agreement with some analyses of the Hubble Deep Field. Four "dr
opout" galaxies are detected at z approximate to 3.8 and are compact in the
IR, similar to 0.5 kpc h(-1) at rest frame 3500 Angstrom. No example of a
blue IR-luminous elliptical galaxy is found, thus restricting the star form
ation epoch of elliptical galaxies to z greater than or equal to 5-10 for a
standard initial mass function and modest extinction.