The galaxy presents irregular stellar and gaseous morphologies. Tschoke et al.
(2001) revealed the presence of a faint, narrow spur of star formation regions
to the South, pointing towards NGC 4569. This spur is also seen in the FP field.
A weak rotation is evidenced in the perturbed velocity map (~100 km s^-1^ in
In Arp 076
Dwarf companion of NGC 4569 at 6.0 arcmin
IBm (de Vaucouleurs)
Paired with UGC 07786 at 6.0, 166
No nucleus. Partially resolved core or bar: 1.4 arcmin x 0.4 arcmin. Faint,
asymmetric, outer extensions.
Pair with NGC 4569 at 6.0 arcmin, possibly interacting.