  We present a comprehensive analysis of a Transiting Exoplanet Survey
Satellite (TESS) high-quality light curve for a young brown dwarf, MHO~4 having
spectral type M7.0, in the Taurus star-forming region. We investigate the
rotation periods and characterize the BD's dynamic atmosphere and surface
features. We present light curve analysis of MHO~4, and estimate the rotation
period to be around 2.224~d. Remarkably, MHO~4 exhibits two significant flaring
events. Furthermore, we also estimated bolometric flare energies to be within
the energy range of $10^{34}$ to $10^{35}$ erg, which sits in the superflare
category.
