The galaxy appears to be a single, relatively smooth object with a generally elliptical morphology. The light profile is centrally concentrated, showing a bright core that gradually fades towards the outer edges. The overall color is yellowish-orange, suggesting a population of older stars and a limited amount of ongoing star formation. There is little indication of spiral arm structure or significant dust lanes. No evidence of tidal tails or significant morphological distortions indicative of major merger events are visible, but some minor asymmetry cannot be ruled out.
