The galaxy presents a complex morphology, exhibiting characteristics suggestive of both smooth and potentially disturbed structures. The overall color gradient indicates a possible transition between an older stellar population toward the central region and more recent star formation activity within some visible features.

The shape appears to be somewhere between round and elongated. There may be some minor disturbances, although these are not strongly pronounced, possibly hinting at interactions or internal processes affecting the galaxy's structure. A dominant, smooth central component with a noticeable color contrast suggests ongoing or recent activity.
