The galaxy presents a generally elliptical morphology. The light is concentrated towards the center, exhibiting a strong central bulge. There is minimal visible disk structure, although a slight flattening is noticeable along one axis. The color gradient suggests older stellar populations dominate, with a yellowish-white hue in the core transitioning to a bluer periphery. There is no obvious sign of active star formation regions or dust lanes, but there is a general hazy blue glow indicating there may be ongoing star formation. The galaxy appears relatively undisturbed, showing no significant signs of tidal interactions or recent mergers and is fairly round.
