  We calculated physical and orbital properties for 2M06464003+0109157, a 1.06
day eclipsing double lined spectroscopic binary. We modelled the system's
ASAS-SN and TESS light curves, measuring the system's inclination and radii of
each component. Extracting radial velocities for each component from 6
SDSS/APOGEE spectra, we measured the system's mass ratio and performed a full
orbital fit. Our analysis indicates that 2M06464003+0109157 has components with
nearly equal masses ($m_1/m_2 =0.99 \pm 0.01$; $M_1{_,}{_2} = 0.57 \pm 0.015$
M$_\odot$) and comparable radii ($R_1 = 0.66 \pm 0.05$ R$_\odot$, $R_2 = 0.57
\pm 0.06$ R$_\odot$). The solution required two star spots to incorporate the
out of eclipse variation that is seen in the light curve. We report our full
characterization of this system, and prospects for similar analyses using
survey data to measure precise physical and orbital properties for EBs.
