The galaxy presents a morphology that appears to be undergoing a merger event or gravitational interaction. Two distinct luminous regions are visible, both with a bluish hue indicative of ongoing star formation, particularly of younger, hotter stars. These regions are somewhat compact and possibly represent the cores of the interacting galaxies. A more diffuse, fainter structure connects the two brighter regions, showing areas of yellow to red colors. This suggests a region of older stellar populations, dust, and possibly gas that is being compressed due to the interaction. The overall shape is irregular and elongated, further supporting the hypothesis of a galaxy merger in progress, as a stable, disk-like or elliptical morphology has not yet been established.
