The galaxy appears to be a relatively smooth, centrally concentrated object. Its light profile suggests a dominant bulge component. The core is bright and yellowish-white, indicating an older stellar population. Fainter, bluer extensions on either side of the bulge may indicate the presence of faint spiral arms or a disk component, although these are not sharply defined. There appear to be some slight disturbances, such as asymmetrical light distribution, but they are minor. The galaxy's overall color suggests it has a moderate amount of ongoing star formation.
