The galaxy presents as a fairly symmetrical elliptical, exhibiting a bright, concentrated core region surrounded by a more diffuse halo. The overall color appears slightly blueish-white, suggesting a population of relatively young, hot stars, although dust may obscure the true color. The galaxy exhibits a nearly circular shape with a slight elongation along one axis. There is no apparent presence of spiral arms or a distinct disk structure. The smooth, symmetrical morphology suggests a relatively relaxed system, likely resulting from the merger of smaller galaxies in the past.
