The galaxy presents as a yellowish-orange, centrally concentrated object. Its morphology appears largely smooth and elliptical, with a high degree of circularity. There is a subtle suggestion of disk-like structure, potentially indicating a spiral galaxy seen at an oblique angle or the presence of a bulge component. Faint, asymmetrical extensions are present, hinting at minor tidal interactions or disturbances. The central region exhibits a brighter concentration of luminosity, likely corresponding to the galactic nucleus. The galaxy displays a moderate redshift, consistent with a relatively high cosmological distance. The overall color suggests an older stellar population, with reduced recent star formation.
