The galaxy presents as an elliptical morphology with a smooth, diffuse light profile. The central region exhibits a concentrated, bright core, suggesting a relatively high stellar density. A subtle color gradient is observed, with the core appearing more yellow-red, indicating an older stellar population, while the outer regions are slightly bluer, perhaps indicating younger stars or ongoing, albeit low levels of star formation. There is no clear evidence of spiral arms or distinct dust lanes. The overall structure appears undisturbed, showing no signs of major mergers or tidal interactions. There may be minor morphological disturbances.
