This galaxy exhibits a morphology consistent with an ongoing merger event. The system presents as a somewhat irregular, extended object rather than a well-defined single galaxy. There are two distinct, brightened regions, suggesting the cores of two galaxies in close proximity. These cores exhibit a yellow-orange hue, implying an older stellar population. Faint bluish tails or arcs appear to emanate from the primary regions, possibly indicative of tidal interactions between the merging galaxies, and suggestive of recent star formation stimulated by the merger. The overall shape is elongated and somewhat disturbed, which strengthens the hypothesis of a merger in progress. The system displays a moderate degree of central concentration of light.
