The galaxy presents as a merging system. Two distinct galactic nuclei are apparent, one displaying a more diffuse morphology and a slightly bluer hue, while the other is more compact and exhibits a redder color. The overall shape of the system is irregular, suggesting ongoing gravitational interactions. There is no obvious spiral structure. Based on its apparent color and morphology, the galaxy is likely an elliptical or lenticular type galaxy undergoing a major merger. This merger system has a high likelihood of triggering elevated star formation, though there is a lack of prominent blue star forming regions.