The galaxy presents as a relatively smooth, elongated structure. It appears to be an elliptical galaxy, likely with a dominant bulge component, indicated by the centrally concentrated light. The shape is cigar shaped with a large fraction of the galaxy being smooth. The light distribution suggests a radial decrease in stellar density away from the center. There is no apparent spiral arm structure, and the overall color is yellowish indicating an older stellar population. There are no major mergers occurring in the galaxy.
