The galaxy presents as a relatively smooth, elliptical morphology with minimal discernible substructure. The light profile appears centrally concentrated, suggesting a prominent bulge component. Color gradients across the galaxy are subtle, with a slightly bluer hue in the outer regions compared to the core, which could indicate ongoing star formation. There is no evidence of a distinct disk, spiral arms, or a recent major merger event from visual inspection. The galaxy exhibits a generally rounded shape, showing only a slight elongation. It shows only a minor chance of a merger or disturbance. Overall, the appearance indicates a more evolved system, potentially a massive elliptical galaxy with a considerable stellar mass and suppressed star formation activity.
