The object presents as an elliptical galaxy with a smooth, featureless morphology. The light distribution indicates a centrally concentrated bulge with a diffuse outer halo. The overall shape is elongated, deviating somewhat from a perfect sphere. There appears to be a slight color gradient from a more yellow/orange core to a slightly bluer halo, which could indicate an older stellar population in the core and a younger population in the outer regions, though this color difference is subtle. No signs of spiral arms, dust lanes, or active star formation regions are apparent in this imagery. The object does not appear to be undergoing any major mergers or tidal disturbances, though there might be very subtle asymmetries.
