The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. Its color gradient suggests an older stellar population, with a yellow-orange core transitioning to slightly bluer hues in the outer regions. There is a general lack of distinct spiral arm structures or prominent dust lanes, suggesting it is likely an elliptical galaxy. The outer regions show a somewhat irregular shape, but no obvious signs of a major merger event. A slight asymmetry is visible, potentially indicative of a minor interaction or past merger event. The overall structure is relatively compact with a smooth profile, but slightly disk-like.
