The galaxy presents a flattened, disk-like morphology with a prominent central bulge. The bulge exhibits a yellowish hue, indicative of an older stellar population. Fainter spiral arm structures extend from the bulge. The disk appears relatively smooth with some indications of patchy star formation activity along the arms. There is a slight asymmetry in the overall structure, which could be a result of a minor gravitational interaction or internal disturbances. The galaxy exhibits a red shift of approximately 0.109, indicating that it is a reasonably distant object. The overall light profile suggests it is a massive galaxy.
