The galaxy presents a disturbed morphology, possibly indicative of a recent or ongoing merger event. There appears to be two distinct, bright nuclei with asymmetrical structures, suggesting the coalescence of two separate galaxies. The overall shape is elongated and irregular. The primary color is yellow-red, with a hint of blue. The overall light distribution indicates a relatively red population. The presence of two distinct light concentrations suggests two galaxies, in either a later stage merging process, or perhaps simply interacting. The internal structure is diffuse, but appears to have a somewhat symmetrical form, with smooth light distribution. The galaxy shows no strong spiral arm features. There is no distinct bulge. The galaxy exhibits overall low levels of star formation activity.
