The galaxy exhibits a morphology suggestive of a late-stage merger or a system undergoing significant tidal disruption. The central region presents a bright, compact core, likely a bulge component, surrounded by a more diffuse halo of light. Faint tidal features, potentially stellar streams or debris, are apparent extending away from the main body of the galaxy. These features appear asymmetric, indicating an ongoing interaction or recent merger event.

The overall color distribution suggests a mixed stellar population. The central region is dominated by yellowish hues, possibly indicative of older stars or a higher concentration of dust. The outer regions exhibit bluer tints, perhaps signifying regions of more recent star formation. The disturbances exhibit hints of blue light, which could also point to star formation. There appear to be a few darker dust lanes obscuring some of the light. 

Given the disrupted morphology and color variations, this galaxy appears to be actively evolving.
