The galaxy presents a largely smooth and elliptical morphology. It displays a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The galaxy appears to be relatively symmetrical, lacking any obvious strong tidal features or major disturbances indicative of recent mergers, though a very slight asymmetry cannot be ruled out. Color gradients are present with a yellowish core, suggesting a population of older stars, transitioning to slightly bluer hues in the outskirts, which may indicate some ongoing, low-level star formation. Overall, the galaxy's appearance suggests a passively evolving system, likely an elliptical galaxy with a moderate mass.
