The galaxy presents an elongated, irregular morphology. There is a dominant central concentration of light with an overall reddish hue, suggesting an older stellar population. Adjacent to this central region, a bluer component is visible, potentially indicating recent star formation activity. The galaxy appears to be undergoing some form of interaction or disturbance, indicated by the overall shape. Evidence suggests a merger is potentially in its final stages, with a clear central bulge, one side appearing more defined than the other.
