The galaxy presents a complex morphology suggestive of an ongoing or recent merger event. It exhibits a generally ellipsoidal form, yet displays notable irregularities in its light distribution. Two prominent, relatively bright, and somewhat compact regions are visible within the galaxy's central area; these may represent the cores of the merging galaxies. These regions appear yellowish, indicating an older stellar population. The fainter outer regions show a blueish hue, suggestive of more recent star formation. The galaxy displays an absolute magnitude indicating a luminous galaxy, however, the specific star formation rate is low, hinting that star formation is either suppressed or has largely ceased. The spatial distribution of light within the system shows a somewhat smooth structure. A third body is also present that appears more red than the other two bodies. 
