The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, centrally concentrated luminosity profile. There is minimal evidence of spiral arms or significant disk structure. The galaxy appears to be moderately round in shape. Its color is relatively uniform across its extent, suggestive of a stellar population dominated by older stars. The overall structure indicates a relatively evolved system. There are no obvious signs of ongoing mergers or major tidal disturbances in the immediate vicinity, although a potential minor asymmetry or disturbance cannot be ruled out. The galaxy is characterized by moderate star formation activity and significant mass.
