NGC 5173. This galaxy shows an extended emission in the MIR distributed
in a smooth way and peaked at the center. HST observations show a high
filamentary structure in the core of this galaxy (van Dokkum & Franx
1995). From its SED (Fig. 4) we see prominent dust excess over the
Pair with NGC 5169 at 5.5 arcmin
E0: (de Vaucouleurs)
See UGC 08465
Non-interacting pair with NGC 5169 at 5.5 arcmin.
All dimensions are for the bright part only.