The galaxy presents an elliptical morphology, appearing mostly smooth with a subtle deviation from perfect sphericity. It exhibits a moderate axial ratio, displaying an intermediate shape between a completely round and a cigar-like form. There are no clearly discernible spiral arms or a pronounced disk structure. The galaxy's light profile indicates a concentrated central region, suggesting a high degree of bulge dominance.

Color gradients are apparent across the galaxy, with the core exhibiting a more yellow or golden hue, possibly indicative of an older stellar population. The outer regions show a slight shift towards bluer colors, hinting at the presence of some younger, hotter stars. The overall color distribution is relatively smooth, without strong evidence of active star-forming regions or dust lanes.

There are no obvious signs of a major ongoing merger. However, subtle irregularities in the outer halo may suggest past interactions or minor disturbances.
