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High quality $gr$ photometry is presented, from which a color-magnitude diagram is constructed, and estimates of age, [Fe/H], [$\\alpha$/Fe], and distance are derived. The star cluster, which we designate as Kim 2, lies at a heliocentric distance of $\\sim105$ kpc. With a half-light radius of $\\sim12.8$ pc and ellipticity of $\\epsilon\\sim0.12$, it shares the properties of outer halo GCs, except for the higher metallicity ([Fe/H]$\\sim-1.0$) and lower luminosity ($M_{V}\\sim-1.5)$. 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