The galaxy presents a morphology that suggests an ongoing or recent interaction or merger event. Two distinct luminous cores are observed, indicating the possible presence of two galactic nuclei. These cores exhibit different colors, with one appearing more yellow-orange and the other having a bluer hue, suggesting differing stellar populations or dust content. The overall light distribution of the galaxy is diffuse and lacks well-defined spiral arms or a prominent bulge. There are tidal features extending from the main body, indicating gravitational interaction. A significant portion of the galaxy's light is concentrated around the two cores, while a fainter, less structured envelope surrounds them. The color gradients across the galaxy suggest variations in star formation activity or dust extinction across different regions. The galaxy's visual characteristics point towards a dynamic system likely undergoing morphological transformation.
