The observed galaxy exhibits a spiral morphology, with a discernible disk structure. Two primary spiral arms are clearly visible, emanating from a central bulge. The arms appear moderately wound, with a mixture of tight and medium pitch angles along their extent. There is no apparent bar structure within the central bulge region. The bulge itself appears relatively small compared to the overall size of the disk. Based on the visible characteristics, a merger is not readily apparent, though there may be minor distortions present within the spiral arm structure. A relatively high number of spiral arms is possible.
