The galaxy presents an elliptical morphology with a smooth light distribution. The light appears concentrated towards the center, exhibiting a characteristic bulge. Two central bright objects, possibly galactic nuclei, suggest a merger event or a binary supermassive black hole system, which would account for the disturbed morphology. The tidal features observed, along with a less luminous object near the main body, further support the theory of an ongoing or recent galactic merger. The color is yellow, possibly indicating an older stellar population with suppressed star formation activity.
