The galaxy presents as a relatively compact object with a somewhat irregular morphology. The central region exhibits a higher surface brightness and a bluish-white hue, indicating the presence of a substantial population of hot, young stars and potentially ongoing star formation. A slightly detached region of similar color appears as a fainter component to the southwest of the primary body, which could indicate tidal disruption, recent interaction with another galaxy, or an independent star-forming region. A disturbed morphology cannot be ruled out. The overall size is moderate, consistent with a system of intermediate mass.
