The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, exhibiting a gradual decrease in luminosity from the core to the outer regions. There is a slight deviation from perfect circularity but it maintains a generally rounded shape. There is a subtle suggestion of a disk-like structure although not very distinct. The light distribution indicates that the galaxy is likely a relatively mature system, possibly undergoing a low level of star formation. There is no obvious evidence of ongoing major mergers or significant tidal disturbances.
