The galaxy presents an elongated, disk-like morphology, viewed at a high inclination, close to edge-on. A prominent central bulge, exhibiting a yellowish-white hue, dominates the galaxy's core region. The bulge appears relatively smooth and concentrated. Fainter, blueish-white light extends away from the bulge along the major axis, suggesting a flattened disk structure.

The disk displays some degree of asymmetry, with a possible warp or tidal feature visible at one end. There is evidence of ongoing star formation, indicated by a patchy distribution of reddish-pink regions within the disk. These regions likely correspond to HII regions, sites of active star birth. Overall, the galaxy presents a complex morphology, indicative of potential interactions or internal processes influencing its structure and star formation activity.
