The galaxy presents as a spiral galaxy exhibiting tightly wound spiral arms. A bulge of moderate size is visible. The disk is inclined relative to our line of sight, appearing somewhat elliptical. The galaxy displays no strong evidence of a central bar structure. The arms appear tightly wound around the central bulge. There's a smooth distribution of light within the galaxy. No signs of significant tidal disturbances or ongoing merger events are discernible. The color profile suggests a dominant stellar population in the redder wavelengths. 
