The galaxy presents a flattened, disk-like structure, indicative of a spiral galaxy viewed at a relatively high inclination. A prominent central bulge dominates the inner region, appearing bright and relatively smooth. Spiral arms are discernible extending from the central bulge, displaying a tightly wound morphology. Evidence of a bar-like structure is visible across the central region. The disk exhibits a range of colors, with a noticeable blue component in the spiral arms suggesting ongoing star formation. There is also a yellow-white hue throughout the galaxy. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers, although minor disturbances cannot be ruled out. The lack of a substantial dust lane supports the galaxy being observed at an angle where dust obscuration is minimized.
