The galaxy presents as a somewhat amorphous, centrally concentrated structure. The core exhibits a yellowish hue, possibly indicative of an older stellar population or dust obscuration. Extending outwards from the core are fainter, bluish wisps and extensions. These could signify regions of more recent star formation. The overall shape appears largely spheroidal, though with some suggestion of asymmetry or possible tidal features. There appears to be some minor disturbance in the morphology. The galaxy lacks well-defined spiral arms, but some structure is observed. The object's red shift places it at a considerable distance, which is consistent with a high luminosity galaxy.
