  We present a high spatial resolution optical and infrared study of the
circumnuclear region in Arp 220, a late-stage galaxy merger. Narrowband imaging
using HST/WFC3 has resolved the previously observed peak in H$\alpha$+[NII]
emission into a bubble-shaped feature. This feature measures 1.6" in diameter,
or 600 pc, and is only 1" northwest of the western nucleus. The bubble is
aligned with the western nucleus and the large-scale outflow axis seen in
X-rays. We explore several possibilities for the bubble origin, including a jet
or outflow from a hidden active galactic nucleus (AGN), outflows from high
levels of star formation within the few hundred pc nuclear gas disk, or an
ultraluminous X-ray source. An obscured AGN or high levels of star formation
within the inner $\sim$100 pc of the nuclei are favored based on the alignment
of the bubble and energetics arguments.
