The galaxy presents a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in brightness outwards from the core. There is a dominance of older stellar populations as indicated by the overall reddish-yellow hue of the galaxy. The absence of well-defined spiral arms or significant dust lanes suggests that this galaxy is likely an elliptical galaxy with minimal ongoing star formation. There does not seem to be any indication of any major disturbances or other galactic interactions occurring.
