The galaxy presents as a spiral structure with a prominent central bulge. The bulge appears yellowish-white, indicative of an older stellar population. Spiral arms are apparent, displaying a range of star formation activity as indicated by the presence of blue regions. The arms appear moderately wound, with several arms being visible, giving the galaxy a multi-armed appearance. Dust lanes are not clearly defined but their presence is weakly implied by subtle obscuration in the spiral arms. The overall color suggests an intermediate-type spiral galaxy, neither strongly blue nor strongly red. No obvious signs of major merger activity are present, although there might be minor disturbances visible. The galaxy exhibits a certain degree of ellipticity.
