The galaxy presents as a single, somewhat amorphous object with no immediately apparent spiral structure. The central region exhibits higher luminosity, indicative of a galactic bulge or core. Extending from this brighter central area are diffuse, fainter regions which may be indicative of tidal features or possibly disturbed morphology suggesting past interaction with another galaxy. The color distribution across the galaxy is not uniform. The core region appears generally more reddish/yellowish suggesting an older stellar population. The fainter, extended regions show a hint of blue, possibly indicating regions of more active star formation. There are also indications of merger activity. Further analysis is required to fully classify the morphology and to ascertain the nature of any interactions.
