The galaxy presents as a somewhat amorphous structure with a slightly elongated shape. It displays a distinct blue hue, suggesting the presence of relatively young, hot stars and ongoing star formation. The light distribution appears uneven, indicating variations in stellar density or dust obscuration within the galaxy. There are regions where the blue light is more concentrated, potentially marking areas of intense star formation. It seems to be experiencing some form of disturbance, indicated by its irregular shape, possibly due to a recent or ongoing interaction with another galaxy. There is no obvious central bulge or spiral arm structure, lending credence to its classification as an irregular or perhaps a disturbed spiral. Evidence of potential merging is supported by the galaxy's chaotic appearance.
