This galaxy appears to be a relatively smooth, elliptical system. The light profile is centrally concentrated, with a gradual decline in surface brightness moving outward. The core region exhibits a yellowish hue, indicative of an older stellar population, which implies minimal present-day star formation activity. The galaxy is generally rounded in appearance with no strong evidence of spiral arms or significant dust lanes. Slight color gradients are present across the galaxy. There are some minor disturbances possibly indicative of recent or ongoing interactions, but the galaxy largely remains undisturbed. Overall the galaxy has a smooth and undisturbed morphology.
