3C 449; z=0.017

The NICMOS image of this galaxy shows the dust lane detected with WFPC2 by [Martel et al.1999] although with less dramatic features. The dust lane has been modeled as a warped disk by [Tremblay et al.2006]. We also detect the abundant globular clusters seen in the optical. The galaxy is elongated north-south and occupies a large portion of the NIC2 chip.