The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. Moving outward from the core, the color shifts toward a slightly redder tone, potentially indicating a mix of stellar populations. The isophotes appear relatively undisturbed, lacking prominent spiral arms or irregular features. Overall, the galaxy appears to be a massive system, with minimal signs of recent or ongoing major mergers.
