The galaxy presents as a spiral type, exhibiting well-defined spiral arms. There are two dominant spiral arms that appear to originate near the galactic center and extend outwards. The central bulge displays a moderate size relative to the overall disk. A bar structure is present, running through the center. The disk is not seen edge-on but is observed at a moderate inclination. There are no obvious signs of a major merger, though some minor disturbances might be present. The galaxy color is yellowish, suggesting a relatively old stellar population and moderate star formation activity. The spiral arms have a medium winding.
