The galaxy presents as a relatively smooth, elliptical morphology. It displays a concentrated central bulge region that gradually diffuses outwards. The core exhibits a bright, yellowish-white luminosity, indicating a potential concentration of older stellar populations. Moving outward from the core, the galaxy shows a subtle transition to a slightly redder hue, although the overall color remains relatively uniform. No prominent spiral arm structures or dust lanes are visible. The outer regions appear somewhat fainter, suggesting a lower stellar density in the galactic halo. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy at a considerable distance.
