The galaxy presents a primarily smooth and concentrated light profile, suggesting an elliptical morphology or a spiral galaxy viewed face-on with a dominant bulge. The central region exhibits a bright, yellowish hue, indicative of an older stellar population. The outer regions of the galaxy appear fainter and slightly bluer, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation in a disk or outer halo component. Overall, the galaxy appears relatively undisturbed, without prominent tidal features or strong signs of recent major merger events. The isophotes seem generally regular and concentric, lending further credence to the classification as an early-type galaxy or a bulge-dominated spiral.
