The galaxy presents as a single, relatively smooth object. The light profile appears concentrated with a bright central core that transitions gradually into a fainter halo. The overall shape is approximately circular, exhibiting a high degree of radial symmetry. There is minimal evidence of spiral arm structures or significant dust lanes. Subtle color variations are present, with a slightly bluer tinge towards the center and redder hues in the outer regions. No signs of tidal tails or strong gravitational disturbances are apparent. The galaxy lacks fine-grained detail, suggesting a lack of prominent star-forming regions or clumpy substructures.
