The galaxy presents a generally smooth, elliptical morphology. It is observed to be largely featureless, exhibiting a high degree of central concentration of light. The light profile gradually decreases from the bright core, and it is quite round in shape. There is no evidence of spiral arm structure or a prominent disk component, and no visual signatures indicating any ongoing or recent major merger events. Faint hints of asymmetry may be suggestive of minor interactions. Color gradients reveal a redder central region gradually transitioning to a bluer halo, consistent with an aging stellar population.
