The galaxy presents as a moderately luminous object, exhibiting a generally smooth, elliptical morphology. Its core region appears significantly brighter, with a yellowish hue that suggests an older stellar population. The extended halo displays a bluer tint, indicating the presence of younger stars and possible ongoing, albeit subdued, star formation. There is little evidence of spiral arm structure or significant dust lanes, further supporting its classification as an elliptical galaxy. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The overall shape deviates slightly from perfectly round, trending more towards an in-between, somewhat flattened, ellipsoidal form. Minor asymmetries or subtle features might be present upon closer inspection with higher resolution data, but are not readily apparent in this image.
