This galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. The primary body of the galaxy appears diffuse and somewhat elongated, with a dominant blue hue suggesting active star formation regions. There is a distinct component with a more concentrated, yellowish glow located nearby which could be a separate galaxy merging with the larger galaxy. The tidal features or extended arms are not well defined, but subtle asymmetries are visible, hinting at gravitational interactions. The system lacks a clearly defined nucleus or spiral arm structure, pointing toward either an early stage in its evolution or the disruptive influence of the merger.
