The galaxy exhibits a morphology consistent with a spiral galaxy, showing distinct spiral arm structures. These arms are tightly wound, tracing a clear pattern emanating from the central bulge. The bulge itself appears moderately sized, with a relatively high concentration of light. Dust lanes are visible within the spiral arms, particularly along their inner edges, giving them a somewhat patchy appearance. The overall color of the galaxy suggests ongoing star formation, indicated by bluer regions within the arms. There are indications of a possible bar structure crossing through the bulge. Furthermore, the galaxy's overall shape appears elongated, with an ellipticity suggestive of a tilted disk. Some visual disturbances are apparent, indicating possible interactions or ongoing mergers.
