The galaxy presents as an edge-on spiral. A prominent central bulge, appearing smoothly elliptical, dominates the structure. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. The disk is thin and elongated, with a higher surface brightness concentrated near the mid-plane. There is little to no indication of resolved star formation regions, which contributes to the galaxy's smooth appearance. The disk appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers. The system presents a high likelihood of residing a substantial distance away. Overall, the object resembles a quiescent, edge-on spiral galaxy with a substantial bulge component.
