The galaxy presents as a largely featureless, elliptical form. It exhibits a smooth, concentrated light profile, suggesting an older stellar population dominating its composition. The central region is bright and yellow-white, indicative of a dense concentration of stars. There is a slight elongation, but it appears mostly spheroidal. No distinct spiral arms or dust lanes are apparent. Very subtle blue fringes are present suggesting a very low level of recent star formation. No major distortions or tidal tails are visible, implying that it hasn't experienced a major merger recently, though some mild disturbance cannot be ruled out.
