The galaxy presents as a diffuse, elliptical-like structure with a smooth overall appearance. It exhibits a centrally concentrated luminosity profile, with the core region appearing brighter than the surrounding areas. The galaxy's color suggests an older stellar population, dominated by redder hues. There is no apparent disk or spiral arm structure visible. The galaxy's shape is more elongated than circular but not extremely so. No evidence of ongoing major mergers or significant tidal disturbances are readily apparent in the image. The galaxy appears relatively isolated, with no closely interacting companions easily discernible.
