The galaxy presents a primarily disk-like morphology, though the structure exhibits some degree of irregularity. A central bulge is visible, appearing relatively smooth and concentrated. The disk exhibits features suggestive of spiral arm structure, albeit somewhat disturbed or flocculent. There is evidence of ongoing or recent star formation activity, indicated by the presence of bluer regions interspersed throughout the disk, possibly tracing regions of active star formation. Some asymmetry in the overall shape is noted, suggesting a potential interaction or past merger event. Some dust lanes may be present across the galaxy.
