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Irregular clumps of emission linked to star formation are
detected in the ultraviolet image of this galaxy [Allen et al.2002].
The near-infrared image shows a flattened galaxy elongated southeast
to northwest. The dust lane perpendicular to the elongation of the
galaxy is visible in both the WFPC2 and NICMOS images. An arc-like
source is present approx.
to the southeast.
David James Elford Floyd
2007-07-28