Spatial mapping of Virgo Cluster members that are neither part of the VCC, the CGCG, nor an additional extended source from NED. The positions of M 49 and M 87 are shown for reference. Three globular clusters are identified from the NGVS and one from NED. The six UCDs from Boselli et al. (2011) and nine UCDs from Brodie et al. (2011) are also shown. Although we currently find low statistics for GCs and UCDs in Virgo from the literature, ongoing spectroscopic studies (e.g., Peng et al., in prep.) are expected to find larger samples of these sources. Thus, we highlight in this figure that the brightest GCs and UCDs are detectable in the UV, and future studies can be performed with upcoming larger samples.