This galaxy presents a largely smooth, elliptical morphology, appearing nearly circular in shape. The central region exhibits a bright, concentrated luminosity profile, likely indicative of an older stellar population and significant mass concentration. The color appears generally redder, especially within the core, suggestive of evolved stars. There is a subtle color gradient towards the outer regions of the galaxy, transitioning to a slightly bluer hue, which hints at a small amount of ongoing or recent star formation, albeit at a low rate. No prominent spiral arms or disk-like structures are visible, and there are no readily apparent signs of recent major merger events or tidal disturbances affecting the overall structure. Faint extensions or features are also not visible, adding to the smoothness of its visual signature.
