The galaxy presents as a spiral system, although the disk's structure is somewhat diffuse. There is the suggestion of spiral arms, but they are not sharply defined, giving the galaxy a slightly flocculent appearance. The galaxy exhibits a slight bulge component, which is of moderate prominence, and is not overly dominant in terms of size. The overall color of the galaxy is consistent with a spiral type, exhibiting bluer hues in the disk regions likely due to younger stellar populations. There's no indication of any major ongoing mergers or tidal disturbances, and the overall form suggests a relatively settled morphology. From the orientation, it appears that the system is being viewed face-on. It is difficult to discern if a bar-like structure is present.
