Many studies of void galaxies’ properties, including optical spectra and photometry, have been published (e.g., Popescu et al., 1997, 1999; Grogin & Geller, 2000; Hogg et al., 2004; Rojas et al., 2005; Collobert et al., 2006; Patiri et al., 2006; Wegner & Grogin, 2008; Hoyle et al., 2012). Combined with H I surveys (Szomoru et al., 1996; Huchtmeier et al., 1997; Kreckel et al., 2011a, 2012, 2015; Ricciardelli et al., 2014; Moorman et al., 2014, 2015, 2016; Douglas et al., 2018), this has resulted in a general consensus that the lower density environments within which the void galaxies reside has only a small effect on their properties. KPNO International Spectroscopic Survey (KISS; Salzer et al., 2000; Gronwall et al., 2004b), which consists of a narrow survey strip that crosses through the void. Several previous studies have considered the metallicities of void galaxies (e.g., Peimbert & Torres-Peimbert, 1992; Cruzen et al., 2002; Kreckel et al., 2015; Douglas et al., 2018), with the latter two studies focusing primarily on dwarf galaxies. Our primary result is that there are no significant differences in the metallicities or the star-formation rates between the KR2 galaxies located in higher density regions and those found in voids

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