226067 was a gas-rich dwarf galaxy [@Beccari16b]. AGC 226067 is projected onto the ‘Low Velocity Cloud’ region of the Virgo Cluster [at $D$$\approx$17Mpc, which we use throughout this work; @Boselli14], which has a velocity distribution centered at $v_{LSR}$$\sim$0 km s$^{-1}$ with a range of $\pm$400 km s$^{-1}$. For simplicity, we refer to the entire system (consisting of the main and secondary stellar bodies, along with the two HI clouds) as AGC 226067 throughout this work, and will refer to particular regions of the system (e.g. its ‘main’ and ‘secondary’ body) when getting into specifics. In addition to a presentation of the [*HST*]{} data (Section \[sec:datareduce\]) and an analysis of the stellar population of AGC 226067 (Section \[sec:props\]), we perform an initial optical/UV archival search for similar stellar systems (Section \[sec:search\]) in deep Virgo cluster data. We discuss possible origins for AGC 226067 in Section \[sec:discuss\], and then conclude (Section \[sec:conclude\]).

[*Hubble Space Telescope*]{} Observations & Data Reduction {#sec:datareduce}
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HST observations of AGC 226067 (GO 13735; PI Sand) were taken with ACS [@ACS] in the F606W (2196 s) and F814W (2336 s) filters on 2015 April 26, as well as the Wide Field Camera 3 (WFC3) in the F275W filter 