The galaxy appears to be a complex system, potentially interacting or merging with a smaller companion. The primary galaxy exhibits a disturbed morphology. There is some evidence of a disk structure, although it appears warped or disrupted. A region of bright, possibly ongoing, star formation is apparent. The galaxy is a moderate redshift, and based on its luminosity, it appears to be a medium-mass system. The presence of a possible merger indicates a relatively low star formation rate relative to its mass, suggesting a possible quenching scenario. The interaction has induced minor tidal disturbance and merging fraction.
