The galaxy presents a prominent disk structure, viewed at an oblique angle. Evidence suggests the presence of spiral arms, although the viewing angle complicates definitive identification. The central bulge appears relatively small and not particularly luminous, and the galaxy shows a generally low surface brightness. The galaxy exhibits a slight central condensation, which may point to a small active galactic nucleus or a centrally concentrated stellar population. The spiral arms, if present, are not tightly wound, suggesting a flocculent or grand-design morphology. Some localized regions of bluer color are visible within the disk, potentially indicating areas of recent or ongoing star formation. The overall shape appears relatively undisturbed, and I do not see any indication of major mergers or tidal interactions. There is only a minor disturbance. Overall, the galaxy appears to be a relatively quiescent spiral galaxy with ongoing star formation.
