The galaxy presents a primarily smooth, elliptical morphology. Its color appears to be generally redder, suggesting a population of older stars and lower current star formation rate. There is some indication of asymmetry or minor disturbance, potentially from a past or ongoing interaction with a smaller object or a minor internal disruption, as there seems to be a slight extension or unevenness in its overall shape. The galaxy displays a relatively concentrated central region, which graduates into a more diffuse halo. There's a subtle color gradient across the galaxy, becoming slightly bluer towards what appears to be an edge, which would indicate some spatial variation in stellar populations or dust content. The morphology is more consistent with an early-type galaxy that has undergone some form of gravitational interaction or internal evolution.
