The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. The core appears bright and somewhat yellow. The galaxy gradually fades in intensity from the core outwards, transitioning to a more indistinct halo. There is a slight elongation to its shape, deviating marginally from a perfect circular form. Overall, the galaxy's structure indicates characteristics of a relatively evolved system, lacking any prominent spiral arms or major disturbances. Faint hints of disk-like structures are observed, although not strongly defined. The color suggests that the stellar population is dominated by older stars, and dust is likely present, but not significantly obscuring the overall view.
