  We are conducting a large program to classify newly discovered Milky Way star
cluster candidates from Froebrich et al. (2007). Here we present NIR follow-up
observations of FSR0190 (RA=20h05m31.3s, DEC=33deg34'09" J2000). The cluster is
situated close to the Galactic Plane (l=70.7302deg, b=+0.9498deg). It shows a
circular shape, a relatively large number of core helium burning stars -- which
clearly distinguishes the cluster from the rich field -- but no centrally
condensed star density profile. We derive an age of more than 7Gyr, a
Galactocentric distance of 10.5kpc, a distance of 10kpc from the Sun, and an
extinction of A_K=0.8mag. The estimated mass is at least of the order of
1E5M_sun, and the absolute brightness is M_V<=-4.7mag; both are rather typical
properties for Palomar-type globular clusters.
