The galaxy presents an elliptical morphology, appearing relatively smooth and concentrated towards its center. The light distribution indicates a substantial bulge component. Color gradients are subtle, transitioning from a yellowish core to slightly redder hues in the outer regions, potentially indicative of older stellar populations dominating the central region. A slight asymmetry in the light distribution is observed, potentially hinting at minor gravitational interactions or internal dust structures. Overall, the galaxy appears to be a relatively quiescent system with low recent star formation activity and a likely high stellar mass. The effective radius indicates the galaxy is of a moderate size.
