The galaxy presents a predominantly smooth and rounded morphology, indicative of an elliptical galaxy. The central region is concentrated, exhibiting a yellow hue, suggesting an older stellar population. A faint, diffuse extension is present, displaying a bluer color, which implies the presence of younger stars, or potentially ongoing star formation. The overall structure appears relatively undisturbed, showing no obvious signs of recent major merger activity, although a minor gravitational interaction may be occurring. The galaxy exhibits a moderate redshift. This points to a location distant from our own galaxy. The overall mass is substantial, estimated to be over ten to the tenth power solar masses. Star formation is present, but is subdued compared to starburst galaxies.
