The galaxy presents a flattened, disk-like structure with a noticeable bulge. There is evidence of a disk or arm-like feature, though the resolution obscures detailed morphology. The galaxy exhibits a gradient in color, with a central region appearing brighter and bluer and the outer regions appearing redder. The overall smooth appearance with signs of disturbance suggest the possibility of interaction or merger. The presence of a central bulge indicates that it could be a spiral galaxy.
