The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The overall shape approximates a sphere, displaying a high degree of roundness. There is a distinct lack of any apparent spiral arm structure or significant morphological disturbances indicative of a major merger event. The color profile suggests an aging stellar population, with a noticeable redder hue in the central regions, transitioning to slightly bluer tones towards the outer halo. This color gradient may indicate ongoing, albeit limited, star formation in the outer regions. Overall, the galaxy appears as a relatively undisturbed system, exhibiting properties consistent with a well-evolved elliptical galaxy that has undergone significant quenching of its star formation activity.
