The galaxy presents as a centrally concentrated, luminous object with a generally smooth morphology. Its overall shape appears elliptical, with a high degree of symmetry. A bright, compact core dominates the galaxy's center, suggesting a substantial concentration of stars and potentially a supermassive black hole. Moving outward from the core, the light gradually fades, indicating a decrease in stellar density. There's a subtle color gradient from the center outwards, where light is more blue. There's no clear evidence of spiral arms or a distinct disk structure and there are only minor signs of any recent or ongoing merger activity. Overall, the galaxy gives the impression of being relatively evolved and quiescent.
