  We quantify the mean asymmetry of 54 face-on, early type disk galaxies (S0 to
Sab) using the amplitude of the m=1 azimuthal Fourier component of the R-band
surface brightness. We find that the median lopsidedness, (A_1/A_0)_{mean}, of
our sample is 0.11 and that the most lopsided 20% of our galaxies have
(A_1/A_0)_{mean} >= 0.19. Asymmetries in early type disks appear to be of
similar frequency and strength as in late type disk galaxies (Zaritsky and Rix
1997.) We have observed our early type disks in a bandpass (R-Band) in which
the light is dominated by stars with ages greater than 10^9 yrs, and therefore
are seeing azimuthal asymmetries in the stellar mass distribution. The similar
degree of lopsidedness seen in disks of very different star formation rates
indicates that the lopsidedness in all galactic disks is primarily due to
azimuthal mass asymmetries. Hence, 20% of all disk galaxies (regardless of
Hubble Type) have azimuthal asymmetries, (A_1/A_0)_{mean} >= 0.19, in their
stellar disk mass distribution, confirming lopsidedness as a dynamical
phenomenon.
