The galaxy presents a generally elliptical morphology, appearing largely smooth and spheroidal in shape. Its core region exhibits a bright, concentrated luminosity, suggesting a significant stellar density or active galactic nucleus. Fainter, diffuse light extends outwards from the central core, indicating a surrounding halo or envelope of stars. There is a slight asymmetry, with a hint of a potential tidal tail or minor disturbance on one side, though its overall structure appears relatively undisturbed. Color gradients are visible, with the central regions trending towards warmer, yellowish hues and the outer regions cooler, with a hint of reddish color. This potentially indicates differences in stellar populations or dust content between the core and periphery. The small angular size suggests it is a distant object, consistent with its estimated redshift.
