The galaxy presents a relatively smooth, centralized light distribution. Its overall morphology appears to be elliptical, exhibiting a high degree of roundness in its shape. There is no clear indication of spiral arms or a pronounced disk-like structure. The galaxy's light profile decreases gradually from the center outwards, with no obvious signs of major disturbances or ongoing mergers. A minor asymmetry may be present in the outer regions, potentially indicating a past interaction or disturbance. Color analysis suggests the galaxy is bluer in the center and appears to shift redder as it fades into the surrounding darkness.
