The galaxy appears to be a relatively smooth, elliptical galaxy with an approximate effective radius of 8.9 kpc. The central region exhibits a strong concentration of light, transitioning into a more diffuse halo. Color gradients suggest an aging stellar population dominating the galaxy's light output, with a subtle blue tinge in the outer regions, possibly indicating recent star formation. The galaxy appears largely undisturbed, lacking strong tidal features or signs of a major merger event. The overall morphology suggests a mature system with ongoing, albeit potentially low-level, star formation activity.
