The galaxy appears to be in the midst of a merger or significant interaction. One distinct component presents a relatively smooth, rounded morphology, appearing largely undisturbed. Adjacent to this is another, smaller component, also relatively smooth in appearance. Between these two components, there is evidence of tidal features, specifically faint streamers or bridges of material linking them. The larger component shows a slightly elongated shape, perhaps indicative of ongoing tidal distortion or a disk structure viewed at an angle. There might also be faint evidence of internal disk structure. Overall, the system exhibits a moderate level of star formation, suggested by the bluish colors.
