The galaxy presents a largely smooth morphology, appearing elliptical in shape. Its light is concentrated towards the center, forming a bright, unresolved core. A diffuse halo surrounds the core, fading gradually into the background sky. There is only faint indication of any distinct spiral arm structure or dust lanes within the galaxy's disk, suggesting that it may be an early-type galaxy with a relatively quiescent star formation rate. The galaxy appears relatively undisturbed, showing no obvious signs of recent or ongoing major merger activity. Faint disturbances may exist on the outskirts of the galaxy, possibly indicating minor interactions with nearby objects. 
