The observed galaxy exhibits a complex morphology, strongly suggestive of an ongoing or recent merger event. The galaxy appears to have two distinct, bright nuclei, each surrounded by a diffuse halo of light. These nuclei display a yellowish hue, potentially indicating an older stellar population or significant dust obscuration. There is evidence of tidal features, such as faint extensions or distortions in the outer regions, further supporting the merger hypothesis. The overall structure appears relatively compact, despite the ongoing interaction. There does not seem to be strong evidence of recent or ongoing star formation.
