The galaxy exhibits a spiral morphology with a clear disk structure. The spiral arms are loosely wound, and appear flocculent, with hints of ongoing star formation. There is a noticeable central bulge region, which presents a moderate contribution to the overall galactic light. The presence of a bar structure is subtle but may exist across the center. The disk is not seen edge-on, and is closer to face on. There appear to be no significant merging events or major disturbances. Overall, it is a rather typical spiral galaxy.
