The galaxy presents a flattened, elliptical morphology. Its central region exhibits a high degree of luminosity with a yellow-white hue, suggesting a concentration of older stellar populations. The luminosity decreases gradually outwards from the core. There is a very slight hint of a disk-like structure, with faint extensions visible along the horizontal axis. The overall color profile shifts towards redder tones in the outer regions. No prominent dust lanes or active star-forming regions are readily apparent. The galaxy shows no indications of major tidal disturbances or ongoing mergers.
