galaxies in the Local Volume [e.g. @Giovanelli10; @Adams13], several searches have been undertaken to characterize their optical properties [@Bellazzini15; @Tollerud15; @Sand15; @Janesh15]. These searches have yielded only a handful of plausible dwarf galaxy counterparts to the UCHVCs, while followup HI observations of others suggest that some may be ‘Dark’ systems [e.g. @Adams16]. Most, however, are likely Galactic HI clouds.

The subject of this paper is [*Hubble Space Telescope*]{} ([*HST*]{}) imaging of AGC 226067 ($v_{\odot}$=$-$140 km s$^{-1}$; also referred to as SECCO1), a UCHVC with an intriguing optical counterpart. First identified by @Bellazzini15, it was confirmed spectroscopically to be associated with the coincident HI cloud [@Bellazzini15UCHVC; @Sand15]. Follow-up high-resolution HI observations with the Very Large Array (VLA) showed that AGC 226067 broke up into two distinct HI clouds [@Adams15] – the primary HI source is coincident with the optical/UV counterpart, while the secondary HI component also has an optical/UV counterpart offset by 0.5’. Data from the Multi Unit Spectroscopic Explorer (MUSE) at the VLT revealed 38 separate HII regions scattered throughout the main and secondary stellar body of AGC 226067, with a nearly uniform metallicity of $\langle$12 + log(O/H)$\rangle$ = 8.37 (for the main body), more metal-rich than expected if AGC 