[*HST*]{} imaging of the UCHVC AGC 226067, an enigmatic gas-rich stellar system in the Virgo cluster. The [*HST*]{} data reveal an exclusively young stellar population of $\sim$7–50 Myr and a \[Fe/H\]$\sim$$-$0.3, in contrast to normal dwarf galaxy systems which always show some old stellar population ($\gtrsim$5 Gyr) upon close inspection. Based on these [*HST*]{} results and other results in the literature on this object (see discussion in Section \[sec:discuss\]), there is circumstantial evidence that AGC 226067 is a distant star-forming remnant of the ram pressure stripping event in the M86 subgroup, as recent simulations have predicted [@Kapferer09; @Tonnesen12].

Our initial search for objects with similar optical/UV properties in the NGVS turned up two objects in 20 deg$^2$, but it is likely that we are only sensitive to the youngest and most luminous examples of this emerging class of stellar objects. Followup HI, X-ray and H$\alpha$ observations of AGC 226067 and its potential brethren will help elucidate their physical nature.

D.J.S. is supported by NSF grants AST-1412504 and AST-1517649. K.S. acknowledges support from the Natural Science and Engineering Research Council of Canada. E.A.K.A. is supported by TOP1EW.14.105, which is financed by the Netherlands Organisation for Scientific Research (NWO). E.T. and P.G 