The galaxy presents as a face-on spiral, exhibiting well-defined spiral arm structure. The arms appear flocculent and moderately wound, possibly three in number. The central bulge is prominent but not overwhelmingly dominant, representing a moderate fraction of the galaxy's overall light. The overall morphology is relatively undisturbed, showing no obvious signs of major mergers or significant tidal interactions. The disk is not edge-on, presenting a clear view of its spiral structure. A weak or no bar structure is present. The galaxy shows evidence of active star formation, but at a relatively moderate rate, with a disk component contributing to a small fraction of its light.
