The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, suggesting a concentration of older stellar populations. The outer regions display a gradual decrease in luminosity, transitioning to a bluish tint, which may indicate the presence of younger stars, though the blue color is very mild and could also come from the redshift. No prominent spiral arms or distinct features are visible; there may be minor dust lanes or disturbances in the outskirts, but they are very faint. Overall, the galaxy presents as a relatively relaxed system, possibly an early-type galaxy nearing the end of its star formation period. The absence of major tidal features or companion galaxies nearby suggests it is not currently undergoing a significant merger event.
