The rms of the residuals in the calibrations are 0.031 and 0.027 mag in V and R respectively. For the host galaxy we measured and in an aperture of radius . The dereddened magnitudes of the host are and . We measured the total AB magnitude of the host galaxy on the CL and LP images in an aperture of radius . The zero points of Gardner et al.
North is up and east is to the left.
The lowest contours are shown linearly whereas the inner contours are logarithmic in order to better show the properties of the host over a large dynamic range. The possible companion galaxy is located near the southern edge of the image. The contour intervals are the same as for Fig.