The galaxy presents a moderately smooth morphology with some visible features. It has an approximate effective radius of 17 kpc. The galaxy appears to be a single object, though some of the structure suggests the possibility of minor disturbances or interactions. It has a redder appearance at the core and becomes blue at the edges. This hints at older stellar populations towards the center, and areas of ongoing star formation on the periphery. There is the possibility that the galaxy may be undergoing a merger or close interaction. The light profile is consistent with a luminous galaxy at a significant cosmological distance.
