This galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape with no discernible disk or spiral arm structures. The central region exhibits a higher surface brightness, gradually decreasing towards the outer edges, lacking defined boundaries. A slight color gradient is observed, shifting from yellowish-green in the core to a more reddish hue in the outskirts, which could be indicative of differential stellar populations and ages, suggesting possible ongoing or recent star formation in the core. There is no apparent evidence of tidal tails or significant distortions suggesting recent major mergers or interactions, appearing as a relatively isolated system. The overall roundness suggests a classification leaning towards an E0 or E1 elliptical galaxy type.
