The galaxy presents as a relatively smooth, centrally concentrated object. There's a noticeable bulge in the center, appearing almost spherical in form. The outer regions of the galaxy appear less defined, with a gradual decrease in brightness moving outwards from the core. There may be subtle hints of a faint disk, but the overall appearance leans toward an elliptical galaxy morphology. There are no obvious signs of major disturbances or a recent merger event, though minor asymmetries cannot be ruled out at this resolution. The galaxy displays a bluer hue in the central regions transitioning to redder tones in the outskirts, hinting at potentially younger stellar populations concentrated within the core, with older, redder populations dominating the outer regions.