The galaxy exhibits a dominant central bulge, appearing relatively smooth and concentrated. It presents a yellowish-white hue indicative of an older stellar population. A faint, diffuse disk surrounds the bulge, subtly extending outwards. There is little indication of significant spiral arm structure or intense star formation regions within the disk based on visible light. Slight irregularities in the outer disk suggest potential minor gravitational interactions or disturbances. Overall, the galaxy displays a rounded morphology leaning towards an elliptical or S0 classification, with only subtle features hinting at a more disk-like nature.
