The galaxy appears to be an elliptical galaxy. It is centrally concentrated, with a smooth, diffuse light distribution. The core region shows a yellowish-white hue, potentially indicating an older stellar population. Moving outward, the galaxy fades into a greenish halo, possibly signifying the presence of a younger stellar population or active star formation. There is some evidence of a slight disturbance in the galaxy's shape. It is slightly elongated, suggesting a possible ongoing or recent merger event. There is also the presence of a small amount of dust. Overall, this appears to be a massive galaxy that is potentially in the process of merging with another galaxy.
