The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central region. A diffuse halo of light extends outwards, with a slight elongation. Color variation is present, with the central region exhibiting a warmer, reddish-orange hue, potentially indicating older stellar populations or dust obscuration. Moving outwards, the halo transitions to a cooler, greenish tint, possibly suggesting a more dispersed population of younger stars or different elemental compositions. There is a hint of a possible minor disturbance or asymmetry in the outer regions. The overall morphology points towards a massive galaxy with a relatively low ongoing star formation rate.
