The galaxy presents as an elliptical structure, elongated with an apparent cigar shape. The core exhibits a bright, concentrated luminosity. Surrounding the core, a more diffuse halo of light is observed, subtly fading towards the outer edges. The overall color profile suggests a population of older stars, possibly with ongoing low-level star formation. There is no strong visual evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no major signs of recent or ongoing mergers, though minor disturbances are possible. The overall form suggests an evolved system, likely with a substantial stellar mass.
