The observed galaxy exhibits a clear spiral structure. Two prominent spiral arms emanate from the central region, displaying a moderate winding. The arms are traced by regions of bluer light, indicating populations of younger, hotter stars and active star formation regions. The central bulge appears relatively small. The galaxy disk dominates the overall light distribution, displaying a generally flat morphology when viewed from our angle. There's no immediately obvious sign of major interaction or recent merger activity.  A bar structure seems to extend through the bulge. The galaxy is exhibiting very little current star formation.
