The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform across the galaxy, suggesting a lack of significant spiral arm structure or prominent dust lanes. The color gradient transitions from a yellowish core to a slightly redder halo, which may suggest a population of older stars dominates throughout. There is a slight elongation to the shape, deviating from perfectly spherical. Evidence of any recent major merger events is not visually apparent, though minor disturbances can’t be ruled out. Based on its smooth features, the galaxy is likely an elliptical galaxy.
