The galaxy presents as a single, relatively smooth object with a high degree of radial symmetry. The light distribution is concentrated towards the center, with a bright core that gradually fades into the surrounding halo. There is no apparent spiral structure or distinct disk component discernible in this image. The galaxy appears quite round, with no obvious elongation. There are hints of color variation, with the central region appearing more yellowish-white and the outer halo showing slightly bluer tones, suggesting differing stellar populations. Overall, the galaxy appears undisturbed, with no evidence of recent mergers or tidal interactions.
