The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a subtle color gradient, with a slightly bluer core transitioning to redder outer regions, suggesting potential variations in stellar populations or dust content. The overall appearance indicates a relatively evolved system, possibly with ongoing, albeit modest, star formation activity. While the bulk of the galaxy seems undisturbed, a very subtle asymmetry in the light distribution may hint at minor past interactions or internal dynamics. No prominent tidal features or strong morphological disturbances are immediately apparent.
