Hierarchical models suggest that galaxies form through a series of mergers that create spheroids of stars, while disks of gas and stars grow around these spheroids during the quiet times between galaxy encounters.  This picture has been questioned in light of the fact that many spiral galaxies have disky "pseudobulges" rather than dynamically hot, spheroidal classical bulges.  I will present "smoking gun" evidence that disk regrowth occurs, and I will show results suggesting that outer disk growth may occur in tandem with pseudobulge growth via frequent episodes of gas inflow and central star formation enhancement. This process may subsume a merger-formed spheroid within a larger disk+pseudobulge system.