The galaxy presents as a luminous, centrally concentrated object. Its morphology appears largely smooth and elliptical, lacking prominent spiral arms or a distinct disk structure. The light profile appears to be nearly round, with a very slight elongation. Color gradients across the galaxy suggest a stellar population that is redder towards the core, indicating older stars, and potentially bluer in the outer regions, which could indicate the presence of younger stars or ongoing star formation. Overall, the galaxy appears to be relatively undisturbed, without any signs of major mergers or tidal interactions. The smooth profile and color distribution suggest a galaxy dominated by an older stellar population.
