The galaxy appears to be of elliptical morphology, displaying a generally smooth light distribution. The radial light profile suggests a moderate concentration of stars toward the center. There is an absence of spiral arms or a prominent disk structure. The dominant color of the galaxy is redder, implying an older stellar population and/or significant dust content. There may be some ongoing star formation, however, indicated by bluer regions. Overall, the galaxy presents as a quiescent system with a moderately high mass. There appears to be some form of minor disturbance event or possible merger with another galaxy. 
