The galaxy presents as an elliptical morphology with a high degree of central concentration. It appears largely smooth in structure, with no obvious spiral arms or distinct features. The core exhibits a bright, yellowish-orange hue, likely indicative of an older stellar population and minimal ongoing star formation. The outer regions of the galaxy show a gradual decrease in brightness, transitioning to a more greenish-tinged halo. This color difference may suggest a slight variation in stellar populations or dust content between the core and the surrounding areas. There is no visible evidence of any major mergers or significant tidal disturbances in the immediate vicinity of the galaxy.
