The galaxy presents as a flattened elliptical, with a smooth, centrally concentrated light distribution. The core region appears bright and yellowish, indicative of an older stellar population. The outer regions exhibit a bluer hue, possibly signifying some ongoing star formation, albeit at a relatively low rate. There are no distinct spiral arms or other prominent features such as dust lanes or tidal tails visible. Overall, the galaxy seems relatively undisturbed, showing no obvious signs of a major merger event. The galaxy appears to be moderately massive.
