The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution without discernible spiral arms or a bar structure. Its color profile suggests a stellar population dominated by older, redder stars, particularly concentrated within the central bulge. There's a subtle color gradient with slightly bluer hues observed in the outer regions, possibly indicating the presence of younger stars or residual star formation at the outskirts. Overall, the galaxy's structure is relatively undisturbed, showing no obvious signs of major mergers or significant tidal interactions.
