This galaxy exhibits a complex morphology suggestive of a possible interaction or merger event. Two distinct, roughly circular, bright central regions are present. Each appears to be surrounded by a more diffuse halo. The light from both halos are of a similar cyan color. The light emanating from both halos seems to consist of a continuum of wavelengths from the green to blue part of the spectrum. The spatial distribution of light is irregular, with no clear spiral arm structure evident. The overall impression is one of significant dynamical disturbance.
