The galaxy presents as a somewhat smooth, centrally concentrated object with a generally elliptical morphology. It exhibits a radial color gradient, appearing more yellowish-white at the core, transitioning to a redder hue in the outer regions. There is no apparent spiral structure or distinct disk component visible. Faint, diffuse features may be present in the surrounding halo, though higher resolution imaging would be necessary to confirm their nature. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of a major merger event.
