This galaxy appears to be an elliptical galaxy, showing a fairly smooth and concentrated light profile. The core is a bright yellow-white, indicating an older stellar population dominating the center. The galaxy exhibits a roughly spherical shape, with a slight ellipticity. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly redder, suggestive of a larger proportion of older, redder stars in the halo. No distinct spiral arms or dust lanes are visible. There is no clear evidence of a recent major merger or significant tidal disturbances in the surrounding stellar distribution. The galaxy exhibits low overall star formation. The observed characteristics indicate a relaxed, relatively evolved system.