The galaxy presents as a generally smooth, elliptical morphology. It exhibits a notable central bulge that is significantly brighter and more concentrated than the outer regions. The color gradient suggests an aging stellar population, with the core appearing more yellow and the outer regions showing subtle hints of bluer hues. The galaxy appears elongated, indicating an elliptical shape deviating from a perfect sphere. There is no obvious presence of spiral arms or a disk structure in the image, further supporting its classification as an elliptical galaxy. Faint, diffuse light extends outwards from the main body, suggesting a stellar halo. There is no obvious sign of a major ongoing merger, although some minor irregularities in the outer structure cannot be ruled out based solely on this image.
