The galaxy presents as a flattened, elliptical shape with a bright, concentrated core. A diffuse, extended halo surrounds the central region, fading gradually into the background. The core exhibits a relatively smooth and uniform texture, suggesting a lack of significant star-forming regions or dust lanes within the nucleus. The surrounding halo appears less uniform, with subtle variations in color and luminosity. Possible minor disturbances in the galaxy's shape and luminosity distribution may indicate tidal interactions or ongoing minor mergers. There is a lack of spiral arm structure. The overall color profile suggests a population of older stars dominating the light output.
