The galaxy presents a generally smooth, elliptical morphology. Its light profile suggests a centrally concentrated spheroid with a gradual decrease in luminosity outwards. The core exhibits a yellowish-white hue, transitioning to a bluer tint in the outer regions of the galaxy. There is no apparent spiral structure or significant dust lane obscuration discernible in the image. Faint, diffuse edges indicate no signs of ongoing major mergers or significant tidal disturbances. The intermediate roundness suggests a shape that is neither perfectly spherical nor highly elongated.
