The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. Two main arms appear to originate near the central bulge and extend outwards, displaying a moderate winding. There is some suggestion of two arms, however, there appears to be splitting in these arms giving the galaxy a more detailed structure. The color distribution shows an overall even distribution of star populations with some younger stars visible in pockets. A slight bar structure may be present but this could be just some asymmetry. The bulge is moderate in size relative to the disk, but not dominant. There seems to be some minor disturbance, potentially suggesting a small interaction or past merger event. The image resolution limits precise classification, but the overall impression is that of a typical spiral galaxy with active star formation, some irregularities that potentially suggest merging and moderate disk.
