The galaxy appears as a smooth, elliptical structure. The central region is bright and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population. The outer regions fade gradually, showing a slight reddish tint, potentially indicating the presence of dust or a lower density of hot, young stars in these areas. No distinct spiral arms or bar features are discernible, supporting the classification as an elliptical galaxy. The overall shape is somewhat elongated, with a length-to-width ratio of approximately 2:1. There is no obvious evidence of recent or ongoing major merger activity or significant tidal disturbances. 
