  The VISTA Variables in the Via L\'actea Extended Survey (VVVX) enables
exploration of previously uncharted territories within the inner Milky Way
(MW), particularly those obscured by stellar crowding and intense extinction.
Our objective is to identify and investigate new star clusters to elucidate
their intrinsic characteristics. Specifically, we are focused on uncovering new
candidate Globular Clusters (GCs) situated at low Galactic latitudes, with the
ultimate goal of completing the census of the MW GC system. Leveraging a
combination of Near-InfraRed (NIR) data from the VVVX survey and Two Micron All
Sky Survey (2MASS), along with optical photometry and precise proper motions
(PMs) from the Gaia Data Release 3 (DR3), we are conducting a systematic
characterisation of new GCs. As a result, we report the discovery and
characterisation of four new Galactic clusters named FSR 1700, FSR 1415, CWNU
4193, and Teutsch 67, all located within the MW disk. We estimate a wide range
of reddening, with values ranging from 0.44 to 0.73 mag for E(J-Ks). The
heliocentric distances span from 10.3 to 13.2 kpc. Additionally, we determine
their metallicities and ages, finding a range of -0.85 to -0.75 dex for [Fe/H]
and ages approximately close to 11 Gyr, respectively. FSR 1415 is an exception,
it is an old open cluster with age = 3 Gyr and [Fe/H] = -0.10. Furthermore, we
fitted the radial density profiles to derive their structural parameters like
tidal radius, core radius, and concentration parameters. In conclusion, based
on their positions, kinematics, metallicities, and ages, and comparing our
findings with existing literature, we categorise FSR 1700, Teutsch 67 and CWNU
4193 as genuine GC candidates, while FSR 1415 is an old open cluster exhibiting
characteristics of a post core-collapse cluster.
