The galaxy presents as a structured object with an apparent red shift. It has a central, concentrated luminosity. There is a disk-like structure, but also indications of either tidal disruption or merging activity. The central region has a yellow-white hue, possibly indicating an older stellar population. Fainter, extended features show a bluer coloration, potentially indicating regions of ongoing star formation. There is a bright object above the main structure that may or may not be associated with the galaxy. The shape is generally round. There is some evidence of a minor disturbance. 
