The galaxy presents as a somewhat amorphous, though generally rounded, structure. Its light profile appears to be smooth with no obvious spiral arms. There is some indication of minor disturbance, with what appears to be at least one other galaxy in the process of merging. The merging has caused a bright central part to appear. This galaxy exhibits colors that tend towards the red end of the spectrum. The median effective radius is on the order of 5 kpc, but because of the disturbance, it may be difficult to accurately discern the extent of the galaxy. The galaxy is not perfectly spherical, as it has a slightly elongated form.
