This galaxy exhibits a complex morphology suggestive of a major merger event. Two distinct luminous cores are apparent, indicating the presence of two galactic nuclei in close proximity. These cores display a relatively smooth, elliptical appearance. A faint bridge of material appears to connect the two cores, indicative of ongoing gravitational interaction. The overall color of the galaxy is yellow-red, possibly due to the presence of older stellar populations. There is a relatively smooth profile and high degree of concentration, with limited evidence of prominent spiral arm structure, despite some blue light present. This suggests a potentially advanced stage of merging where tidal features are present as well as moderate star formation occurring within the remnants.
