The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a nearly circular morphology, with a high degree of central symmetry. The galaxy's light profile appears to gradually decrease in intensity from the core outwards. The color of the core appears to be bluish-white, transitioning to more yellow in the outskirts, suggesting a population of younger stars dominating the central region and older stars comprising the halo. There is no apparent spiral structure or bar. There are no obvious signs of a major merger event or significant tidal disturbances.
