The galaxy exhibits a complex morphology, possibly undergoing a merger or significant tidal interaction. The central region presents a diffuse, smooth component which might be composed of older stellar populations. Extended beyond this is a disturbed, elongated feature that appears to be a tidal tail, potentially originating from a smaller merging galaxy or recent interaction. The color gradient across the galaxy suggests spatial variations in stellar population age and dust content. There are indications of on-going star formation within the tidal feature.
