The galaxy presents a relatively smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that gradually diffuses outward into a less defined halo. The color appears to be predominantly bluish-white, suggesting the presence of a moderate population of younger, hotter stars. The overall structure lacks prominent features such as spiral arms or dust lanes, indicating a more evolved system. There may be some slight asymmetry in the outer halo, hinting at a possible past minor interaction or disturbance, although the galaxy primarily appears relaxed and undisturbed.
