The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Color gradients suggest an aging stellar population, indicated by the redder hue of the core. The outer regions display a fainter, bluer color, potentially indicating more recent, though subdued, star formation activity. The overall morphology appears undisturbed, showing no obvious signs of tidal interactions or recent mergers. The galaxy has a moderately compact size for its estimated luminosity and mass. It shows little evidence of a prominent disk or spiral arms, which is consistent with its classification as a possibly spheroidal or elliptical galaxy.
