The galaxy exhibits a discernible disk-like morphology. The disk component presents with a notable degree of structure, indicating the presence of distinct features. Visual inspection suggests the possibility of a recent or ongoing merger event, supported by morphological disturbances observed within the disk. There are no strong indicators of a substantial spheroidal component. It is possible there are tidal tails visible; there appears to be some disruption near the body of the galaxy.

The galaxy appears to be relatively small in angular size. The color of the galaxy suggests active star formation, as indicated by a brighter magnitude in the r-band compared to the z-band.
