The galaxy presents as a smooth, elongated structure, likely an elliptical or lenticular galaxy, observed at a redshift suggesting a considerable distance. The core exhibits a bright, concentrated luminosity, indicative of a high stellar density. The color profile suggests a primarily older stellar population with a yellowish hue, particularly prominent in the central bulge. Fainter, diffuse blue regions are observed. The overall morphology appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
