The galaxy presents a largely smooth and centrally concentrated morphology. Its overall shape appears elliptical, with the light intensity gradually decreasing from a bright core outwards. The core exhibits a yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the color subtly shifts toward redder tones, particularly in the extended halo region, potentially indicating a greater presence of cooler, evolved stars or dust obscuration. Some subtle irregularities or faint features hinting at a disk-like structure, though this is not the dominant characteristic. No major disturbances or clear signs of an ongoing merger are evident, however there could be minor disturbances.
