The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical with an overall circular shape. There is a slight color gradient, with the core region exhibiting a yellowish hue suggestive of an older stellar population. The outer regions appear slightly bluer, possibly indicating the presence of some younger stars, but the light is dominated by older stars overall. There is no obvious evidence of spiral arms, a prominent disk, or significant dust lanes. No signs of merging or tidal disruption are apparent. The galaxy exhibits a smooth luminosity profile, declining gradually from the central core to the outer edges.
