The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge with a yellow-orange hue, indicative of an older stellar population. There is some indication of a faint, diffuse disk surrounding the central bulge, but without any clearly defined spiral arms or significant features. The roundness appears relatively circular, with an average smoothness. There is no visually discernible evidence of ongoing major mergers or significant tidal disturbances, although there is a minor possibility of a minor disturbance occurring. Based on the red color, it appears to have a very low star formation rate and would be classified as a quiescent galaxy. 
