The galaxy presents a predominantly smooth and rounded morphology. There is a brighter central bulge region, possibly indicative of a supermassive black hole. Faint, extended features appear on either side of the bulge, possibly indicative of a disturbed disk. One side displays a more elongated, plume-like structure, suggestive of tidal interactions with another galaxy, or some other disturbance event. Overall, the galaxy exhibits characteristics that could indicate either an elliptical galaxy with recent minor disturbances, or perhaps a spiral galaxy undergoing a transformation.
