The galaxy presents as a somewhat diffuse object, exhibiting a yellowish-white hue. It is moderately compact. There is evidence of disturbances in the structure, perhaps related to on-going merging events. The galaxy displays an irregular, non-smooth profile. The shape appears somewhat in between round and elongated. There seems to be potentially multiple nuclei or regions of high stellar density. There are hints of disruption beyond the main body of the galaxy. 
