The galaxy appears to be an ongoing or completed merger of two distinct galactic structures. One component presents a relatively smooth, elliptical morphology with a dominant yellowish hue, suggesting an older stellar population and minimal ongoing star formation. The other component exhibits a more irregular shape with regions of bluer light, indicative of younger stars and active star formation. There appears to be some tidal distortion or disruption evident in the bluer regions, possibly caused by gravitational interactions during the merger. The overall size of the interacting system is moderately extended, spanning an estimated 5 kpc.
