The galaxy presents as a largely smooth, elliptical object. It exhibits a bright, concentrated central bulge, transitioning outwards to a more diffuse halo. The color profile shifts from a yellowish-white core to a bluer, fainter outer region. There is little evidence of spiral arm structure or significant dust lanes, suggesting a relatively evolved stellar population. The overall morphology appears undisturbed, with no strong indications of recent major merger events, although subtle disturbances cannot be ruled out. The round shape of the galaxy is noticeable. There might be weak ongoing star formation activity, as suggested by the bluer color in the outer regions, though it appears subdued. Overall, the galaxy seems consistent with a massive, quiescent system with a dominant spheroidal component.
