The galaxy presents as a spiral type, oriented at a near-intermediate angle relative to the observer. The disk is noticeably more prominent than the bulge component. Distinct spiral arm structures are observed, appearing somewhat flocculent and not tightly wound. The arms are of a bluish hue, indicating recent star formation. A moderate bulge is visible, exhibiting a yellowish color, suggesting an older stellar population. Evidence suggests the presence of a small bar structure. The galaxy shows minor disturbances that could possibly be due to a minor merger event.
