The galaxy exhibits a spiral morphology, characterized by a relatively high degree of symmetry and a discernible disk structure. Spiral arms appear present, though somewhat flocculent. The galaxy's central bulge seems comparatively subdued relative to the overall disk luminosity. The spiral arms display a moderate winding, neither tightly wound nor particularly loose. Some indication of a central bar feature is present. The disk itself presents a slight inclination relative to the observer's line of sight, but not edge-on. There seems to be a bit of star formation activity present throughout the galaxy.
