The galaxy presents as a spiral, viewed at a moderate inclination. A central bulge is apparent. The disk shows organized spiral structure, with hints of two dominant arms. The spiral arms appear to be wound somewhat tightly around the central bulge. There is an indication of a bar-like structure crossing the central region. The overall color suggests a mix of stellar populations, with a somewhat redder bulge region and bluer disk. No significant tidal features or signs of major mergers are obvious in this image.