The galaxy presents as a relatively smooth, elliptical-like structure. Its color profile indicates an older stellar population, with a central yellowish hue. The isophotes appear to be generally concentric, though with a slight deviation from perfect circularity, displaying a mild elongation. No prominent spiral arms or dust lanes are discernible in the available imagery. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly bluer, potentially indicating younger stars or lower metallicity in the outskirts. The overall morphology suggests a galaxy that has largely completed its major merging events and is now dominated by evolved stars.
