The galaxy appears to be in the process of merging, or at least undergoing a significant interaction. It has a disturbed morphology, lacking a clear spiral or elliptical structure. Two distinct, bright cores are visible, suggesting the original nuclei of the merging galaxies. These cores exhibit a yellowish hue. Diffuse, fainter material surrounds the cores, with a bluish tinge observed, possibly indicating regions of recent star formation triggered by the interaction. The overall shape is elongated and irregular, with no obvious bar feature. Evidence of tidal tails or extended streams of stars are not obvious in this image, but the disruption of the main bodies indicates a strong gravitational influence.