This galaxy appears to be in a late-stage interaction or merger. It exhibits a complex morphology, lacking a clear single nucleus. The central region is dominated by a bright, somewhat amorphous, yellow-white component, possibly indicative of an older stellar population. Extending outwards, there are fainter bluish-green regions that suggest the presence of younger stars, perhaps recently formed due to the interaction. There are notable disturbances in the overall structure, hints of tidal tails or bridges, and possibly a secondary nucleus. This disruption further suggests a recent or ongoing merger event. Overall, this galaxy appears to be an intermediate-mass system exhibiting moderate star formation activity. The structure is not that of a disk galaxy, it exhibits more amorphous components, not quite like a well-formed elliptical.
