The galaxy presents as a relatively smooth, centrally concentrated object. There is a slight elongation observable, but it appears largely circular. The dominant color is yellowish-white, suggestive of an older stellar population. The presence of a fainter, bluer halo surrounding the central region indicates a younger stellar population and recent or ongoing star formation. Faint, disturbed features are visible in the outer regions, which may indicate that the galaxy is undergoing or has undergone a minor merger event.
