The galaxy presents as a centrally concentrated, luminous object with a generally smooth, elliptical morphology. Its color appears yellow-white toward the core, suggesting a population of older stars dominating this region. There is minimal evidence of spiral arms or significant dust lanes, consistent with a largely spheroidal structure. The outer regions fade gradually, with a subtle transition to a bluer hue, possibly indicating the presence of younger stellar populations at the periphery, although this is not very pronounced. The galaxy exhibits a high degree of central symmetry. Based on the image, there is no obvious sign of active galactic nuclei activity or tidal disturbance from recent mergers. The overall structure suggests an evolved system with a high fraction of early-type stars.
