The galaxy presents as a largely featureless, elliptical morphology. It exhibits a smooth, centrally concentrated light profile, with a high degree of roundness. The core appears bright and yellowish, transitioning to a more diffuse, greenish-blue outer halo. There is no discernible evidence of spiral arms, bars, or active galactic nuclei based on the image. There are no major disturbances or merger signatures evident in the galaxy's structure. The outer regions are not clearly defined, likely due to the low surface brightness and distance. The color gradients suggest a potentially older stellar population dominating the central region, while a younger stellar population is distributed more diffusely within the galaxy. 
