Structural properties of the galaxy LBT1 in relation to low mass galaxies in the Local Group (McConnachie 2012). For its stellar mass, LBT1 has an effective radius which is common within the Local Group satellite population. However, its central surface brightness (μ_V(0) ∼ 26.8 mag arcsec⁻²) is among the faintest for its stellar mass. If LBT1 were in the Local Group it would resemble properties similar to the dwarf spheroidals Andromeda XIV or Sextans.