The galaxy exhibits a generally elliptical morphology, although it appears slightly elongated. The primary light emission is concentrated in a bright, yellowish central bulge. The color suggests a relatively older stellar population dominating the core. There is a subtle suggestion of a disk structure extending outwards from the bulge, oriented roughly horizontally in the image. The disk appears fainter and bluer than the central bulge, which may indicate regions of more recent star formation, though likely at a very low rate. There appears to be a faint asymmetry or minor disturbance on one side of the galaxy, potentially hinting at a past interaction or merger event. Overall, the galaxy presents itself as a relatively smooth, evolved system, dominated by an aging stellar population, with only subtle signs of ongoing activity.
