The galaxy presents a morphology suggestive of an ongoing or recent merger event. Two distinct luminous regions are observed, indicating the presence of two galactic nuclei in close proximity. These nuclei exhibit a relatively smooth, unresolved appearance. The overall shape of the galaxy is somewhat rounded but clearly disturbed, lacking a well-defined spiral or elliptical structure. Light distribution indicates some redder areas, especially in the outskirts, as well as brighter, bluer areas associated with the nuclei. There is an area of less intense luminosity between the two nuclei. The galaxy has some evidence of tidal features or distortions beyond its core regions.
