The galaxy presents as an elongated structure. There is a suggestion of asymmetry in the light distribution along its major axis, where there is a concentration of diffuse light with some blue hue on one side. Fainter redder knots of light are irregularly distributed near the middle. The overall form hints at a possible disturbed morphology. Based on the presence of the blue hue, at least a small population of younger stars are present. There also appears to be a faint reddish halo surrounding the main body of the galaxy. 
