The galaxy presents as a mostly smooth, elliptical-like structure. The light profile suggests a high degree of central concentration, with a gradual decrease in brightness towards the outer regions. There is a slight elongation visible, deviating from a perfect sphere. It exhibits a reddish-yellow hue, suggestive of an older stellar population dominating the light output. No prominent spiral arms or dust lanes are discernible in this image. It appears to be in a relatively quiescent state with low ongoing star formation. There might be a very minor disturbance or interaction visible on its side, but it is hard to tell.