The galaxy presents an elliptical morphology, appearing mostly smooth and well-defined. It exhibits a concentrated central bulge with decreasing luminosity towards the edges. The color profile suggests a population of older stars, with a dominant yellowish-orange hue throughout the galaxy. There is an absence of prominent spiral arms or dust lanes. Faint bluer regions appear. The galaxy appears relatively undisturbed with no obvious signs of a major merger or tidal interactions. 
