The galaxy presents as a spiral type, viewed at a moderate inclination. A central bulge is present, appearing mostly smooth and elliptical in shape. Faint spiral arms can be observed extending from the central bulge, with hints of diffuse structure. The bluer regions are somewhat irregular in shape. There is no clear evidence of strong tidal features or a major ongoing merger event, though minor disturbances cannot be ruled out. Based on the blueness of the outer parts and the presence of star formation one might expect, there could be a modest rate of star formation. The galaxy appears to be a significant mass, with a generally smooth distribution of light.
