The galaxy presents a largely smooth morphology, with an overall elliptical shape, with hints of disklike features. The light is centrally concentrated, with a bright, yellowish core that fades into a bluer halo. There is little evidence of strong spiral arm structure or significant dust lanes. The galaxy appears relatively isolated, showing no clear signs of major interaction or ongoing merger activity, although there is faint, minor disturbance. The relative color suggests a population dominated by older stars with a moderate amount of on going star formation.
