The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a roughly elliptical morphology with a high degree of central light concentration. The color profile suggests a general red-shift, with a subtle shift toward bluer hues in the outer edges of the galaxy. No distinct spiral arm structures or significant dust lanes are visible. The galaxy’s overall structure indicates it's a quite well formed elliptical galaxy. The light distribution is relatively uniform, hinting at a well-mixed stellar population. There appear to be no signs of active galactic nuclei or recent major merger activity, as the galaxy seems relatively undisturbed.
