The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology suggests it is likely an elliptical galaxy, though potentially a lenticular galaxy viewed face-on. The primary color is yellowish-white at the center, suggesting an older stellar population dominates the core. The outer regions exhibit a slightly bluer hue indicating the presence of younger stars, although overall star formation activity appears to be low. There are no obvious signs of spiral arms or a prominent disk. There is no discernible presence of tidal tails, merging signatures, or other strong gravitational disturbances, suggesting this galaxy is likely relaxed and isolated. It is roughly circular in appearance, showing only a very slight deviation from perfect roundness.
