The galaxy presents as a largely smooth, centrally concentrated object. It exhibits a primarily elliptical morphology, with a high degree of circularity. A bright, concentrated core is visible, transitioning into a fainter, more diffuse halo. The color profile indicates a redder core, likely populated by older stellar populations, fading to slightly bluer hues in the outer regions, which could indicate some ongoing, but limited, star formation. There is no clear indication of spiral arms or a pronounced disk structure. Minimal signs of tidal disturbances or interactions with other galaxies are apparent in the immediate vicinity. The galaxy appears to be relatively isolated.
