The galaxy presents as a centrally concentrated, smooth object, most likely an elliptical galaxy. The light is primarily yellow and orange, which may indicate an older stellar population with lower rates of star formation. The isophotes appear largely circular, with only a slight deviation from perfect roundness. It appears that there is some form of tidal disturbance to the lower right of the central body, perhaps a dwarf galaxy that is in the process of merging with the main galaxy. There is no strong evidence of spiral arms or prominent dust lanes. This is consistent with a galaxy that has undergone significant morphological transformation. Overall, the galaxy appears relatively undisturbed aside from the merging occurring to the lower right.
