The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is elliptical in nature, exhibiting a high degree of circularity. The central region of the galaxy appears to be a bright yellowish-white, with the intensity gradually decreasing towards the outer edges. There is a discernible color gradient, transitioning from the warmer hues of the center to cooler, bluer tones in the surrounding halo. This suggests a possible difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars more prevalent in the outer regions. No distinct spiral arms or dust lanes are visible. There are no signs of a major ongoing merger or significant tidal disturbances, but very subtle minor asymmetries or disturbances cannot be ruled out.
