The galaxy presents a largely smooth, elliptical morphology. It is highly concentrated, with a bright, yellowish core that diffuses outward. The outer regions fade gradually, exhibiting a reddish hue. No distinct spiral arms or disk-like features are discernible, although some very subtle, potentially disturbed regions are present. There is no clear evidence of a major ongoing merger, though a minor interaction cannot be entirely ruled out based on the subtle distortions observed. The general shape is close to circular.
