The galaxy presents a largely smooth, elliptical morphology. There is no discernible disk structure. The central region exhibits a bright, concentrated core, with a gradual decrease in luminosity towards the outer edges. The object appears relatively round in shape.

Color gradients are subtle but present. The central region has a more yellow-orange hue, suggesting an older stellar population. Fainter bluish tinges on the outskirts indicate the presence of younger, hotter stars, potentially signaling ongoing star formation in the outer regions of the galaxy.

Based on the observed features, the galaxy is likely a massive elliptical galaxy with a moderate redshift, experiencing a small amount of ongoing star formation. No evidence of major mergers or significant tidal disturbances are apparent in the immediate vicinity of the object.
