The galaxy appears to be in a state of interaction or merger. Two distinct luminous components are visible, suggestive of two separate galactic nuclei. The overall morphology is disturbed, lacking a clear, well-defined structure such as a spiral arm or elliptical shape. The light distribution is relatively smooth within each component, but the connection between the components exhibits signs of tidal distortion or bridging material. The color is generally yellow/orange, which is often indicative of a relatively older stellar population.
