The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. It has an overall oblong shape, neither perfectly circular nor highly elongated. The central region shows a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy appear fainter and slightly bluer, hinting at the presence of some younger, though likely subdued, star formation activity. There is no clear indication of spiral arms or a prominent disk structure. No signs of major ongoing mergers or tidal disturbances are apparent, although a possible slight asymmetry might suggest a minor interaction in its past. The galaxy's overall color and morphology indicate a relatively passive system with a low star formation rate.
