The galaxy presents as a system undergoing a minor disturbance. Its overall form can be classified as an intermediate morphology between smooth and disk-like. The light distribution suggests it is not perfectly round, leaning toward an elliptical shape. The galaxy's central region exhibits a somewhat smooth appearance, but fainter disturbances or irregular features extend from the core. There is some evidence of tidal features. Based on the color indices, there is no strong evidence of ongoing significant star formation, which could indicate it is in the process of becoming a more quiescent system. The galaxy is relatively compact.
