The galaxy presents as a disturbed system, possibly undergoing a merger. The morphology displays an elongated form, neither purely elliptical nor a well-defined spiral. There is a distinct color gradient across the galaxy, with one end appearing more reddish/yellowish and the other presenting a bluer hue. This suggests differential stellar populations, possibly due to ongoing or recent star formation in the bluer region. The galaxy does not appear to be a pure disk, and exhibits features implying it could be the result of a merger event. Evidence indicates that the galaxy does exhibit a low rate of star formation. The disturbance and irregular morphology suggest the possibility of tidal interactions.
