The galaxy presents a flattened, elliptical morphology. It exhibits a smooth, centralized concentration of light, suggestive of an older stellar population. The core region appears reddish, possibly indicating a high concentration of evolved stars and dust obscuration. Moving outward from the center, the galaxy's color shifts toward a more yellowish-green hue. The outer edges of the galaxy gradually fade into the background, exhibiting no sharp boundaries or spiral arm structures within the limitations of the resolution. There appear to be no obvious signs of recent major mergers or significant tidal disturbances.
