The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. The color profile shifts from a yellowish core to a slightly redder halo. No distinct spiral arms or significant dust lanes are visible. The overall form suggests a galaxy undergoing minimal current star formation, consistent with a more evolved stellar population. There is a slight elongation, with the galaxy being more "in between" round and cigar-shaped. There is a noticeable lack of any significant merging activity or major disturbances in its structure.
