The galaxy presents as a singular, largely featureless object. It exhibits a near-spherical morphology. The central region displays a high surface brightness, appearing concentrated and luminous with a yellow hue. The light gradually fades into an extended, less luminous halo. The overall color suggests an evolved stellar population, potentially dominated by older, redder stars, with very little indication of ongoing, active star formation. There is a distinct lack of spiral arms or other significant structures that would indicate a disk galaxy. The absence of morphological disturbance indicates that the galaxy is not currently undergoing a major merger event. 
