The galaxy appears as a centrally concentrated, ellipsoidal object. Its morphology is smooth and relatively featureless, lacking prominent spiral arms or a distinct bar structure. The light profile suggests a concentration of older stellar populations, with a dominant reddish-yellow hue indicative of evolved stars.

The roundness of the galaxy is close to circular, appearing as a near perfect sphere. There is no distinct nucleus and the light gradually diminishes in intensity moving from the center outwards, which suggests that the star formation activity is very low. There is no presence of significant dust lanes, and the color gradient is very smooth. There does not appear to be any evidence of any mergers or disturbances in the galaxy. 
