The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, lacking any prominent spiral arm structures or a distinct, flattened disk. The light distribution exhibits a radial gradient, with a bright, compact core that gradually fades into the surrounding halo. No obvious signs of recent or ongoing major mergers are discernible, the galaxy appears relatively undisturbed. The color profile suggests a population dominated by older stars, with a subtle reddening from the core outwards.
