The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a high density of older stellar populations. Moving outward from the core, the light gradually fades into a bluish halo, potentially indicative of younger stars or lower metallicity. The galaxy appears largely undisturbed, exhibiting no strong signs of ongoing mergers or tidal interactions, though some faint asymmetries in the outer regions cannot be ruled out entirely. Based on the apparent color gradient and overall smooth structure, this galaxy is likely an elliptical galaxy with a moderate redshift.
