The galaxy presents as a somewhat diffuse, elliptical structure. Its color appears primarily reddish, indicating an older stellar population with relatively low ongoing star formation. There is a suggestion of a smoother, more featureless morphology, possibly indicating that it is an elliptical galaxy viewed at a considerable distance. There is evidence suggesting an ongoing merger event; a slightly disturbed structure is visible, which shows the potential interaction with a smaller galaxy. Overall, the galaxy appears relatively massive.
