The galaxy exhibits a complex morphology, with evidence suggesting it is undergoing a merger. The primary body of the galaxy appears relatively smooth, with a subtle concentration of light towards the center, indicative of a possible bulge. The galaxy shows an intermediate ellipticity, being neither perfectly round nor highly elongated. There is a significant distortion or feature suggesting an ongoing interaction. A less diffuse patch appears distinct, potentially signifying an accreting dwarf galaxy or a tidal remnant. There is an indication of star formation activity within the galaxy, noticeable as bluer regions possibly containing younger stellar populations. The system shows signs of disturbance, which could be indicative of a merger in progress.