The galaxy presents a clear spiral structure, with a morphology that is decidedly not smooth. The arms are well-defined and prominent, extending outwards from a bright, moderately sized central bulge. The winding of the spiral arms appears to be of an intermediate nature, neither tightly wound nor exceptionally loose. Distinct segments within the arms suggest the presence of ongoing or recent star formation activity. Two dominant arms are observed. There is no strong evidence of a prominent bar feature bisecting the central bulge, though some evidence for a weak bar may be present. The overall structure seems relatively undisturbed, though some subtle asymmetry is observed. The light distribution shows a moderate concentration towards the central region, indicative of a classical bulge component.
