The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light profile appears to decline gradually from the bright core, showing no evidence of spiral arm structure or a prominent disk. There are no obvious tidal features or other signs of recent major mergers. The color gradient suggests a population of older stars. The galaxy exhibits a largely homogenous texture, lacking significant internal substructure or distinct star-forming regions that might be indicative of ongoing star formation. It is also mostly round in appearance.
