The galaxy presents as a somewhat irregular structure. There is a suggestion of a disk-like component, although it is significantly disrupted. Within this disk, there appear to be several distinct clumps of brighter emission, suggestive of ongoing star formation regions. There may be signs of tidal tails emanating from the central region, giving it an overall disturbed appearance. There are no clear spiral arm structures visible. The galaxy appears to be relatively faint, and its light is shifted slightly towards the red end of the spectrum.
