The galaxy presents a somewhat smooth, elliptical-like morphology with a slight disk-like component. The object displays a central bulge that dominates the overall structure, surrounded by a faint, diffuse halo. There appears to be some level of disturbance with possible interactions or past mergers, as the halo is not uniformly distributed around the bulge and may have some distortions. This galaxy has intermediate mass, with a relatively moderate star formation rate, and displays signs of ongoing or recent interaction, potentially indicative of a system undergoing morphological transformation.
