The object presents as a spiral galaxy, seen at a significant inclination. There is evidence of a disk-like structure, though it is somewhat disrupted and ill-defined. Indications of dust lanes are visible along the central region, suggesting ongoing star formation. The galaxy displays a blueish hue and the overall structure indicates a mass of around 10^10 solar masses. There seems to be some evidence of ongoing or recent interactions with another galaxy, given its somewhat disturbed morphology. 
