The galaxy presents a smooth, elliptical morphology. There is little evidence of spiral arm structure or prominent dust lanes. Its overall shape appears somewhat elongated, but is still fairly close to round. The central region is brighter than the outer edges, indicating a concentration of stars towards the core. There is a slight color gradient from the center outwards, with the core exhibiting a yellow hue. The overall color profile suggests the presence of an older stellar population. There is no evidence of any major ongoing mergers or significant tidal disturbances. The galaxy is mostly smooth and unfeatured, with no notable substructures visible in this image.
