The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that fades into a diffuse halo. The color profile indicates a dominant population of older stars, evidenced by the reddish-yellow hue observed towards the galactic center. There is little indication of spiral arm structure or significant dust lanes. The overall structure suggests a relaxed system, potentially an evolved galaxy which is supported by its smooth shape and lack of disturbance. There might be some evidence of minor interaction or tidal features, but it is not obvious.
