The galaxy presents a primarily smooth and rounded morphology, with an overall elliptical shape. The central region exhibits a high degree of luminosity, appearing bright yellow-white, indicating a dense concentration of stars, likely older stellar populations. Moving outward from the core, the intensity gradually decreases, transitioning to a more diffuse yellow-orange halo, and finally fading into darker colors at its edges. Faint hints of asymmetry or possible tidal features are visible, hinting at minor gravitational interactions, but these are not obviously indicative of a major merger event.
