The galaxy presents a largely smooth, elliptical morphology, with a significant concentration of light towards the center. The color gradient is subtly suggestive of an older stellar population, appearing more reddish in the central regions and subtly trending towards bluer hues in the outer edges. There is no visible structure suggestive of spiral arms or a prominent disk. The overall shape is close to round, but closer inspection suggests it could be slightly in between round and cigar shaped. There are no obvious signs of active merging or major disturbances.
