The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from the central region, displaying a grand design structure. The arms appear loosely wound, extending outwards into the galactic disk. The central bulge is of moderate size in relation to the disk.  There is evidence of a bar structure present, exhibiting moderate prominence. The disk component dominates over the bulge, with the galaxy demonstrating a high rate of star formation. No major signs of mergers are seen, and a small disruption may be occurring in the overall structure, likely to be a minor merging event.
