The galaxy appears to be a likely merger of two distinct galaxies. Both progenitor galaxies are disk-like, with ellipsoidal morphologies and noticeable tidal disturbances. One galaxy appears to be larger than the other. There is a visible difference in color gradient between the central regions and outer edges. The central regions of both galaxies exhibit a reddish hue, possibly indicating an older stellar population. The outer regions are a paler green-blue hue, suggestive of more recent star formation and a younger stellar population. The smoother morphology fraction suggests the overall structure is somewhat homogeneous despite the merger, which is further supported by the colors of the regions blending rather than being distinct.
