The galaxy presents as a centrally concentrated, elliptical-like structure. Its core exhibits a yellowish-white hue, suggesting an older stellar population. The light smoothly decreases in intensity as one observes outwards from the center. Fainter extensions are slightly bluer compared to the core. The galaxy does not display any clear evidence of spiral arms or a prominent disk, instead having a smoother, more amorphous appearance. There are no strong indications of tidal tails or major disturbances due to mergers; although some slight asymmetry or distortion of the outer regions cannot be completely ruled out, but they appear minimal.
