The galaxy presents a morphology consistent with a spiral galaxy, displaying a prominent central bulge. The bulge appears relatively bright, suggesting a concentration of older stellar populations. Faint spiral arms extend outwards from the central region, exhibiting a somewhat flocculent structure. The arms appear to be moderately wound, displaying a mixture of tightly and loosely wound segments. A possible bar feature is present within the central region. The galaxy exhibits an overall blue hue, suggesting ongoing star formation. The disk is not edge-on, and no major merger events seem to be occurring, although there is a hint of minor disturbance. Two spiral arms appear to be present. 
