The galaxy presents a generally smooth and featureless morphology. It appears elliptical in shape, with a high degree of central concentration as evidenced by the bright, yellowish core. There's a slight elongation, suggesting it is not perfectly spherical. The light gradually fades towards the outer edges, indicating a smoothly decreasing stellar density. There are no prominent spiral arms, dust lanes, or signs of active star formation visually discernible within the galaxy's structure. No tidal tails or obvious signs of major mergers are observed, though subtle disturbances cannot be ruled out. The overall color suggests an older stellar population.
