The galaxy presents a dual-core morphology, indicative of a possible ongoing or recent merger event. Each core appears relatively compact and bright, exhibiting a bluish hue. Faint extensions or tidal tails may be present, though difficult to discern from the background noise. The overall structure appears disturbed, rather than exhibiting smooth, elliptical features or well-defined spiral arms. It is likely experiencing interactions. The redder colors indicate older stellar populations.
