The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is quite round. The light distribution suggests a concentration toward the center, with a gradual decrease in brightness as one moves outward. The galaxy exhibits a subtle blue hue, potentially indicative of some star formation, albeit at a relatively low rate. There is no apparent evidence of major disturbances such as tidal tails or multiple nuclei, suggesting that it is not undergoing a major merger event, however there may be minor disturbances. The galaxy appears largely undisturbed.
