The galaxy presents a largely smooth, elliptical morphology with a prominent, centrally concentrated bulge. The bulge exhibits a distinct orange hue, possibly indicative of an older stellar population. A faint, diffuse halo surrounds the core, transitioning to a greenish tint, suggesting a component of younger stars or ongoing star formation, albeit at a low rate. The overall form is generally rounded, with only slight deviations from perfect circularity. There is no strong evidence of major mergers or significant tidal disturbances in the galaxy's structure, although minor irregularities may be present.
