The galaxy presents a disturbed morphology, suggestive of an ongoing or recent merger event. Two distinct, bright nuclei are observed within a common, diffuse halo. The nuclei exhibit a yellowish-white color, potentially indicating an older stellar population. There is very little evidence of recent star formation. The overall shape appears irregular, lacking defined spiral arms or a prominent bulge structure. Faint tidal features or streamers may be present in the outer regions, further supporting the merger hypothesis. The galaxy appears relatively compact in size, with the two nuclei in close proximity.
