The galaxy presents as a somewhat elliptical, though not perfectly circular, structure. The central region exhibits a high degree of luminosity, suggesting a concentration of older stellar populations. There are faint traces of disk-like features but the overall impression is one of smoothness, without prominent spiral arms or distinct structures. Subtle color variations can be observed, hinting at differing stellar populations and possible dust lanes, though the resolution limits a detailed examination. No signs of major mergers are apparent in the image, though there is a chance for minor disturbances.
