The galaxy presents as a centrally concentrated, generally smooth object. It appears to be elliptical in shape, with a high degree of circularity. The core exhibits a bright, yellowish-white luminosity, suggesting a concentration of older stellar populations. Surrounding the core is a more diffuse, greenish-yellow halo. There is very little evidence of spiral arm structure or significant dust lanes. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major recent merger events or tidal distortions. The light profile falls off relatively smoothly from the core outwards, transitioning to a lower surface brightness in the outer regions.
