The galaxy presents as an irregular, extended object with a complex morphology. It appears to be undergoing a significant interaction or merger. There are no obvious spiral arms or a defined elliptical shape. The central region shows a higher concentration of light, suggesting a core or nucleus, although it is not sharply defined. Distinct clumps of varying colors are present. There is a noticeable blue-green area at one edge. The overall color profile suggests a mix of stellar populations, with both older, redder stars, and regions of ongoing star formation, indicated by the blue-green hues. The irregular shape and the presence of distinct, multi-colored clumps strongly imply an active merger event involving at least two galactic components.
