This galaxy presents as a moderately luminous elliptical, appearing mostly smooth and well-defined. The core of the galaxy exhibits a high degree of central concentration, with a gradual decrease in luminosity towards the outer regions. The shape is slightly elongated, exhibiting a mild deviation from a perfect circular form. There is no apparent structure such as spiral arms or a prominent disk, indicating a relatively old stellar population. Subtle color gradients are present, with a slightly bluer hue toward the central regions which would be indicative of some ongoing, although minor, star formation activity. No signs of major disturbances from interactions or mergers are observed.
