The galaxy appears to be an interacting system composed of two distinct components. One component presents a smoother, more rounded morphology with a somewhat elliptical shape. Its light is comparatively homogenous. The second component is more elongated, with a more obvious disk like shape, and exhibits a color that suggests a more active star formation rate. There is a faint, extended halo of light around the two objects, potentially indicating tidal interactions or merger activity between the two galaxies. Overall, this appears to be a relatively compact system undergoing an interaction or merger.
