The galaxy presents a generally smooth and rounded morphology. It appears as a concentrated central bulge with a diffuse, low-surface-brightness halo extending outwards. There is little to no evidence of spiral arm structure or a prominent disk. The light profile suggests an elliptical galaxy or a lenticular galaxy seen face-on. Faint color variations are present, with a somewhat bluer hue near the central region, possibly indicating ongoing, though subdued, star formation. The lack of significant distortions suggests the galaxy is relatively undisturbed, with no recent major mergers or tidal interactions. The overall appearance indicates a galaxy dominated by an older stellar population.
