The object appears to be a system of at least two galaxies undergoing a significant interaction or merger. Both galaxies exhibit a flattened morphology suggestive of disk galaxies. One of the galaxies is viewed nearly edge-on, with a prominent central bulge that has a rounded appearance. There is evidence of tidal tails or bridges of material connecting the two galaxies. The disk of the edge-on galaxy appears distorted, potentially due to the gravitational interaction with its companion. The overall color suggests moderate levels of star formation activity, particularly within the disturbed regions and tidal features. It is plausible that the interaction is triggering star formation. The galaxies appear to be of substantial mass.
