The galaxy presents a roughly elliptical morphology. It appears to be relatively compact. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population density or possibly an active galactic nucleus. A fainter, diffuse halo surrounds the central core. There is some suggestion of minor disturbances or asymmetries in the outer regions, potentially indicative of past or ongoing interactions or mergers. Color gradients are visible, with the central region appearing bluer, possibly indicative of younger, hotter stars, and the outer regions exhibiting a redder hue. The general appearance is more smooth in texture with a possible disk.
