The galaxy presents a generally smooth morphology, with an apparent elliptical shape. The central region exhibits a concentrated, bright core, suggestive of an older stellar population dominating in that area. Extending outwards from the core, there's a noticeable decline in luminosity, gradually fading into the surrounding background. There may be some subtle distortions in the outer regions, possibly indicating past or ongoing interactions with smaller galaxies, or tidal effects. Overall, the galaxy appears relatively undisturbed with a significant spheroidal component.
