The galaxy presents as a centrally concentrated object with an elliptical morphology. The core region exhibits a bright, yellowish-orange hue, suggesting a population of older stars. The outer regions appear to be slightly elongated. There appears to be no distinct spiral arm structure. Subtle color gradients are visible, transitioning from the warmer core to cooler, bluer colors in the outer regions. There are no apparent signs of active star formation or recent merger events. The galaxy is relatively smooth in appearance.