The galaxy presents a largely smooth, elliptical morphology. Its structure is dominated by a centrally concentrated bulge exhibiting a reddish hue, suggesting an older stellar population. Fainter, diffuse light extends outwards from the core, transitioning to greenish-yellow. There is no apparent spiral structure or significant dust lane obscuration evident in this image. The overall appearance indicates a quiescent system with little active star formation. Subtle distortions may be present, though not overtly indicative of a major merger event. The galaxy appears relatively undisturbed.
