This galaxy appears to be a merging system, possibly in the late stages of interaction. The overall structure presents a somewhat rounded morphology, with no clearly defined spiral arms or disk-like features readily apparent. There is an indication of dual nuclei, or two high density concentrations of stars, which supports the classification of this galaxy being in a major merger. The galaxy exhibits an overall smooth appearance, suggesting a relatively even distribution of stellar populations, with redder color indices. The lack of pronounced blue regions may indicate a suppressed star formation rate or a population dominated by older stars. Overall, this galaxy likely represents a significant event in its evolutionary history as two galaxies merge together.
