The galaxy presents as a relatively smooth, centralized structure. It exhibits a near-circular morphology with a high degree of central concentration. The galaxy core emits strongly in bluer wavelengths, suggesting the presence of a population of hot, young stars or possibly an active galactic nucleus. A faint, extended halo with reddish hues surrounds the core, indicative of older stellar populations and potentially dust. There are some signs of minor disturbances. The overall structure suggests an evolved system, though not perfectly spherical.
