The galaxy presents as a spiral type, exhibiting a distinct disk structure viewed at a moderate inclination. The central bulge is prominent but not exceptionally large, appearing somewhat blended with the disk, which is a characteristic of later-type spirals. Spiral arms are readily visible, displaying a grand design, organized and extending outwards from the core. The arms appear tightly wound in some regions and less so in others, displaying regions with possible star-forming activity. Overall, the spiral structure dominates the galaxy's appearance, with a relatively small and weakly barred bulge. There's no strong evidence of ongoing major mergers or significant tidal disturbances. The galaxy exhibits a smooth disk.
