This galaxy exhibits a complex morphology, presenting characteristics of both smooth and featured structures. The central region appears relatively smooth, potentially indicating an older stellar population. However, the outer regions reveal evidence of a disk-like structure, with hints of spiral arms or irregular features. There are also signs of potential disturbances, with some asymmetry. The general color gradient from the center outwards may suggest ongoing star formation in the more external regions. Overall, the galaxy does not appear to be undergoing a major merger.
