The galaxy presents a largely smooth, symmetrical morphology, characteristic of an elliptical galaxy. It exhibits a centrally concentrated light profile, with a bright, yellowish core that gradually fades into the surrounding halo. There is no discernible spiral arm structure, bar, or other distinct features typically associated with disk galaxies. Subtle color gradients are apparent, suggesting potential variations in stellar populations or dust content within the galaxy. There are no apparent tidal tails, bridges, or signs of ongoing major mergers, though subtle asymmetries may suggest minor disturbances.
