The galaxy presents as a single, relatively smooth and elliptical structure. The central region exhibits a bright, concentrated luminosity that fades gradually toward the outer edges. There is a minimal presence of distinct features, such as spiral arms or dust lanes, with the overall light distribution appearing largely uniform and consistent with an elliptical morphology. The galaxy’s round shape suggests minimal recent or ongoing merger activity, with no visual evidence of tidal tails or disturbed structures. The color profile indicates a population of older stars, consistent with a low star formation rate. The apparent size and brightness imply a galaxy of significant mass, which is typical of elliptical galaxies observed at this distance.
