The galaxy presents as a somewhat smooth, centrally concentrated object, approximately elliptical in appearance. The core region exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions display a slightly bluer color gradient, hinting at the presence of younger stellar populations and potentially ongoing, but low, star formation. There is some subtle asymmetry or minor disturbances visible, possibly indicative of a past or ongoing minor interaction or merger event. The galaxy does not show any strong spiral arm structure or a distinct disk. Overall, the galaxy appears to be an early-type galaxy with some signs of activity.
