The galaxy presents as a diffuse, centrally concentrated object. Its morphology appears to be somewhat smooth, although there is evidence of possible disturbances in the overall structure. The primary light distribution is concentrated toward the center, with a more diffuse halo extending outwards. There is some evidence for a complex structure including multiple nuclei, possibly indicative of a galaxy merger in progress. The object is significantly more luminous than other objects in the field. Colors are consistent with a galaxy at moderate redshift.
