The galaxy appears to be a relatively smooth, elliptical system. Its light profile suggests a concentrated central bulge with a gradual decrease in luminosity outwards. It has an approximately round shape and shows a generally even distribution of light, with a slight blue hue in the outer regions. There is no obvious evidence of spiral arms or significant dust lanes. The overall morphology points towards an older stellar population and a system that has undergone significant dynamical relaxation. There seems to be only a minor disturbance, if any, to the overall structure of the galaxy.
