This galaxy exhibits a clear spiral structure. The arms are prominent and somewhat tightly wound around a central bulge. The bulge itself appears relatively small compared to the overall size of the disk. Several HII regions are visible within the arms, indicating ongoing star formation. Some asymmetry is present, with one side appearing more distorted than the other, possibly indicative of tidal interactions or past mergers. The galaxy is not seen edge-on, presenting a clear view of the disk structure. There appears to be a bar feature. The spiral arms are not uniform and their number is hard to tell. There may be a merger event occurring, but the galaxy may also just be disturbed.
