The galaxy presents a primarily smooth morphology. There is some evidence of a disk-like structure and/or faint features, but they are not prominent. The overall shape is roughly in-between round and cigar-shaped, with a slight elongation visible along its major axis. The light distribution is relatively concentrated towards the center. There does not appear to be any major ongoing merger activity, although the possibility of minor disturbances cannot be completely ruled out. The object's light suggests a evolved stellar population with little active star formation.
