The observed galaxy exhibits a morphology consistent with an ongoing or recent merger event. The light distribution presents a disturbed structure, lacking a clear, singular nucleus. Instead, two distinct, bright concentrations are apparent, suggesting the presence of at least two galactic nuclei within the system. 

The overall color profile indicates a mix of stellar populations. The central regions display a yellowish-white hue, suggestive of older, more evolved stars. Fainter, bluer patches are observed peripherally, potentially indicative of regions with ongoing star formation. 

There is faint evidence of tidal tails extending from the main body, further supporting the hypothesis of gravitational interaction and disruption. No obvious dust lanes are discernible. The galaxy's shape is markedly irregular, lacking the defined spiral or elliptical structure expected of quiescent galaxies.
