The galaxy presents a somewhat amorphous structure, appearing elongated with a moderate axial ratio. Its overall color profile is yellowish-orange, suggesting a population of older stars, though some bluer regions are hinted at. There are signs of an ongoing or recent merger event, with potential tidal features or distortions in the outer regions of the galaxy. It doesn't show a clear spiral or barred spiral morphology. The galaxy displays a centrally concentrated light distribution, but with some unevenness, likely due to the interaction. It seems to be actively forming stars at a moderate rate. The galaxy's overall smoothness is relatively high, suggesting it may be transitioning into an elliptical galaxy due to the merger.
