The galaxy exhibits a disk-like morphology but also appears to have an elliptical component. Its central region shows a smooth light distribution. Faint spiral arm structures are visible, though they appear somewhat disrupted or ill-defined. The object has a slight degree of elongation. The galaxy's color suggests that it is populated by a mix of stellar populations. It may also have a small merger occuring. There are hints of an interaction or disturbance in its morphology.
