This galaxy presents as a largely smooth, elliptical morphology. The light is concentrated toward the center, exhibiting a bright, yellowish core which appears to be the galactic nucleus. Moving outward from the core, the light gradually diminishes, transitioning to a more diffuse, bluish halo. The apparent roundness of the galaxy suggests it is viewed relatively face-on. There is no clear evidence of spiral arm structures or major disturbances from ongoing mergers. Some minor asymmetry is seen in the outer edges of the halo.
