The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, largely featureless morphology, with a high degree of radial symmetry. The luminosity profile appears to be dominated by an older stellar population, as suggested by the yellowish-red hue dominating the central region. There are subtle hints of bluer color in the outer regions, potentially indicating pockets of more recent star formation, albeit at a low rate. The galaxy appears relatively undisturbed, with no obvious signs of ongoing or recent major merger events. Faint tidal features are not readily apparent, further supporting the assertion of a dynamically relaxed system. The overall shape is more rounded than elongated.
