The galaxy exhibits an irregular morphology, suggestive of an ongoing or recent interaction or merger event. The light distribution appears clumpy and complex, with multiple bright knots or regions of intense emission. A tidal tail appears to be present, extending along the bottom. There is a distinct region of bluer light present along the top and rightmost region of the galaxy and a dimmer region of light present at the bottom and left. There is a possible interaction with another galaxy. Overall, the structure deviates significantly from a simple elliptical or spiral form.
