The galaxy presents as a centrally concentrated object with an apparent diffuse halo extending outwards. There is evidence of a possible disk-like structure oriented roughly horizontally across the central region. The galaxy's core is intensely luminous and appears to be somewhat rectangular. The shape might be due to the resolution of the instrument. There is a hint of structure outside this core area, the appearance is more likely due to noise. There is a redder patch of light to the left. The object appears relatively isolated.
