The galaxy presents a morphology suggestive of a late-type spiral, possibly undergoing a significant interaction. Two primary spiral arms are discernable, though rather loosely wound, and their structure appears somewhat disrupted. The galactic bulge is moderate in size. It possesses a weak bar structure. Significant tidal distortions are apparent, indicating a possible merger. The central region exhibits a moderately concentrated brightness profile, however the outer disk fades gradually. Star formation is ongoing, as evidenced by the blue color within the arms.
