The galaxy presents an elliptical morphology, appearing smooth and relatively featureless. Its overall shape is somewhat elongated, with an intermediate axis ratio. The central region exhibits a high concentration of light, suggesting a dense stellar population or possibly an active galactic nucleus, though at this resolution the latter cannot be confirmed visually. The light profile seems to gradually decrease from the center outward. There is a subtle color gradient across the galaxy, with the core exhibiting a more yellowish or reddish hue compared to the outer regions, which appear slightly bluer. This could indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars present in the outer parts, though the lack of discernible spiral arms or prominent star-forming regions suggests that star formation activity is low. No signs of any major or minor merger are visible.
