The galaxy presents as a relatively smooth, elliptical object. Its core exhibits a concentrated luminosity, appearing intensely bright and yellowish-white. The light gradually diffuses outward, transitioning into a more reddish hue as it reaches the galaxy's outer edges. This suggests an older stellar population predominates in the outer regions. There is no discernible spiral structure or dust lanes visible. The overall morphology appears undisturbed, with no obvious signs of tidal interactions or recent mergers. The galaxy displays a high degree of circularity in its isophotes.
