The galaxy presents as a generally smooth, elliptical morphology, with a high degree of circularity. No distinct features such as spiral arms or a prominent bar are apparent. There is a slight color gradient from the center outwards, with the core of the galaxy displaying a more reddish/yellow hue, transitioning to a slightly bluer color further out. This may indicate older stellar populations concentrated towards the center and younger, hotter stars distributed more peripherally. The galaxy shows no significant signs of ongoing mergers or major disturbances, with a relatively undisturbed appearance. Overall, the galaxy appears to be a relatively massive, evolved system, with a suppressed star formation rate.
