The galaxy presents as a largely elliptical structure, exhibiting a smooth, symmetrical morphology. There is a high degree of central concentration with a bright, yellowish core suggesting an older stellar population in the galactic nucleus. Surrounding this core is a more diffuse halo, with a subtle color gradient shifting towards cooler blue hues at the periphery, implying the presence of some younger stars or perhaps a higher metallicity gas in the outer regions, but not in significant quantities. There is no apparent disk structure or spiral arm features. The galaxy appears relatively isolated, showing no signs of significant tidal interactions or major disturbances, although there may be minor perturbations to the overall shape. The overall visual impression is that of a quiescent, evolved galaxy.
