The galaxy presents as a smooth, elliptical form with a high degree of central concentration. The overall color appears to be a yellowish-white, suggesting an older stellar population and potentially lower levels of current star formation. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. There is no apparent structure such as spiral arms or a prominent bar. Faint outer regions fade gradually into the background sky. The galaxy is relatively isolated, without obvious signs of recent tidal interactions or major mergers.
