The galaxy presents a generally smooth and rounded morphology. There is very little discernible disk structure, and no major distortions or signs of ongoing mergers are readily apparent. The light distribution appears centrally concentrated. There are no clear spiral arms and the galaxy's color indicates that the galaxy hosts an intermediate population of stars. There is evidence of minor irregular light distribution or faint tidal features which would be consistent with a small disturbance or past minor merger. Overall, the galaxy is a relatively undisturbed, evolved system.
