The galaxy presents as an elliptical morphology, displaying a largely smooth and concentrated light profile. The core region appears bright and yellowish-white, potentially indicative of an older stellar population. There is a subtle color gradient from the center outwards, transitioning to a slightly redder hue. No distinct spiral arms or dust lanes are discernible. The overall shape is approximately circular, with only a minor deviation towards elongation. There is no visually apparent evidence of ongoing merging activity or major disturbances in the galaxy's structure. The smooth, rounded appearance suggests a relatively relaxed and evolved system.
