The galaxy appears to be a relatively smooth, elliptical system. Its morphology suggests a classification as an early-type galaxy. The galaxy exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards its outer regions. There is an absence of distinct spiral arms or prominent dust lanes. The color profile suggests a predominantly older stellar population. There are subtle indications of possible minor disturbances, but the overall structure is largely undisturbed. Its overall shape is fairly round, lacking any significant elongation.
