The galaxy presents as a largely featureless elliptical structure, appearing smooth and concentrated towards the center. The core exhibits a bright, intense luminosity. Moving outwards, the galaxy displays a gradual decrease in surface brightness, with a more diffuse halo. There is a hint of a disk structure, or perhaps spiral arms. Overall, the galaxy is relatively symmetrical in shape, with a slight elongation. It does not obviously show signs of any ongoing major merging activity or tidal disturbances, although a minor disturbance cannot be ruled out.
