Results of a five-month campaign of optical monitoring the Seyfert 1 g
alaxy NGC 4593 are presented. High resolution Halpha and Hbeta spectra
and direct images in the Johnson U, B, V, R and I bands were obtained
between January and June 1990. The emission lines and the continuum s
howed strong variations on time scales of weeks to days. The Halpha li
ne varied by more than 30 % within only 5 days. Cross-correlating the
light curves of the Balmer lines with that of the optical continuum gi
ves a lag of around 4 days. Therefore, this low luminosity Seyfert gal
axy may have one of the smallest BLRs known so far.