This galaxy presents as a well-defined elliptical shape. The central region exhibits high luminosity with a bright, concentrated core, which appears almost spherical. The light gradually fades outward from the center, forming a smooth, diffuse halo surrounding the core. There is a slight elongation to the structure, hinting at a possible mild distortion, though no strong tidal features or prominent dust lanes are immediately apparent. The color profile suggests a population of older stars, giving it a slightly redder appearance in the outer regions transitioning to a bluer hue towards its active center. Overall, the morphology leans towards a relatively undisturbed system, though further spectroscopic analysis would be needed to confirm its kinematic properties and star formation history.
