The galaxy presents as a largely elliptical morphology with a smooth, diffuse appearance. The light profile suggests a high degree of radial symmetry, with a central bulge that appears significantly brighter and more concentrated than the outer regions. The color gradient indicates a redder core, possibly indicative of an older stellar population or increased dust obscuration. A subtle halo surrounds the main body of the galaxy, gradually fading into the background. There is no evidence of spiral arms or significant disk features.
