This galaxy appears to be in the process of a significant merger event. Two distinct luminous components are visible, suggesting either two galactic nuclei or the remnant core of one galaxy interacting with the primary galaxy. One component is more diffuse and brighter with a slightly reddish hue, potentially indicating an older stellar population or significant dust obscuration. The second component is slightly bluer and more compact, possibly indicative of ongoing or recent star formation. There are faint tidal features or distortions, potentially bridges or tails that suggest gravitational interaction between the two components. These indicate the ongoing disruption of their structures. Overall, it appears to be an elliptical or lenticular galaxy undergoing an interaction/merger.
