The galaxy presents as an edge-on spiral with a prominent, centrally concentrated bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. A flattened disk extends outward from the bulge, appearing somewhat diffuse and elongated. The disk shows hints of blueish star formation regions, particularly towards the outer edges, indicating more recent star formation activity. There is some indication of dust lanes running across the disk, although the resolution limits detailed observation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major merger. The luminosity appears relatively high, suggesting that the galaxy is somewhat massive, or a result of recent star formation.
