The galaxy presents as a moderately redshifted system, exhibiting an elongated, cigar-shaped morphology. Its light profile appears relatively smooth, suggesting a higher fraction of older stellar populations. There is a concentration of light toward the central region which is yellow tinted. Fainter diffuse light extends outwards from the core, showing some blue tints at the periphery. The overall structure implies a system that has undergone some disturbance, although it does not show clear signs of a major ongoing merger.
