The galaxy presents as a centrally concentrated object with a smooth light distribution. It appears elliptical in shape. The core exhibits a bright, yellowish-white hue, which suggests an older stellar population. There is a radial decrease in light intensity moving away from the center. A faint, diffuse halo appears to surround the main body of the galaxy. A small, fainter object is detected close to the core and toward the right side of the galaxy. The object does not appear to be strongly interacting with the galaxy, although some disturbance cannot be ruled out. The overall color profile suggests relatively low levels of ongoing star formation.
