The galaxy exhibits a generally smooth morphology, with a centrally concentrated light profile. The object appears to be undergoing a significant interaction or merger. Two distinct luminous regions are apparent, potentially representing the cores of the progenitor galaxies. These regions display variations in color. The primary region displays yellow to red hues, while the secondary region exhibits blue light. This distribution of colors suggests a complex mix of stellar populations and dust content within the merging system. There is some indication of tidal features, potentially faint streams or distortions extending beyond the main bodies of the system, indicative of ongoing gravitational interactions. The galaxy, as a whole, presents an irregular shape.
