The galaxy presents a largely smooth, elliptical morphology. It appears roughly circular in shape, showing little to no discernible disk structure. The light distribution is centrally concentrated, with a gradual decrease in intensity outward from the core. The color profile suggests an evolved stellar population, exhibiting a yellowish-orange hue. No major disturbances or signs of ongoing merger activity are readily apparent. A slight asymmetry is potentially visible, but this could simply be from imaging imperfections. Overall, the galaxy appears to be a relatively undisturbed, quiescent system with minimal star formation activity.
