The galaxy presents as a spiral galaxy undergoing a significant merger event. The central bulge exhibits a concentrated, bright yellowish hue, suggesting an older stellar population and potentially a supermassive black hole actively accreting material. The disk component is visibly disturbed, with asymmetric extensions of light radiating outwards from the main body. One side of the disk appears more disrupted, displaying a bluer color, which may indicate ongoing or recent star formation triggered by the merger. Patches of redder hues are also observed, possibly regions of dust obscuration or older stellar populations within the disturbed disk. There are indications of tidal tails or streams of stars and gas extending away from the main galaxy body, further corroborating the ongoing merger process. Overall, the galaxy appears to be a dynamic system in a state of flux, significantly shaped by the gravitational interactions of the merger.
