The galaxy presents as a flattened disk structure, indicating it is likely a spiral or lenticular galaxy seen at an oblique angle. The central region exhibits a high surface brightness, suggesting a significant concentration of stars, potentially a bulge component. The galaxy's light profile appears relatively smooth with no apparent flocculence. The bluer color of the outer disk, along with detected Hydrogen, potentially indicates areas of active or recent star formation. There is likely little to no sign of a recent major merger event, but a small disturbance cannot be ruled out.
