The galaxy presents as a moderately luminous, early-type system, likely an elliptical or lenticular galaxy, observed at a significant redshift. Its overall morphology appears smooth and relatively featureless, with a high degree of central concentration. The isophotes are generally elliptical, displaying an aspect ratio suggesting some degree of flattening, but with a dominant spheroidal component. The color profile indicates a relatively red population, suggestive of older stars and limited on-going star formation. There's no discernible spiral arm structure or prominent dust lanes visible. Faint extensions could imply minor tidal interactions, though no major merging activity is evident.
