This galaxy presents a disk morphology, viewed at a shallow angle, not quite face-on but not edge-on either. Distinct spiral arm structures are visible. The arms appear relatively loosely wound, extending from the central region. There is evidence of a bar-like structure spanning at least halfway across the galactic center. It possesses what seems to be a central bulge, although not a particularly prominent one. The galaxy displays a blueish color profile, possibly indicative of on-going star formation within its spiral arms. There is some visible distortion or asymmetry in the spiral arm structure, possibly suggesting a minor gravitational interaction. The galaxy appears generally isolated, with no other similarly sized objects appearing to be causing the disturbance. There is no obvious indication of a major merger or tidal tail.