The galaxy presents as a single, somewhat amorphous object with a concentrated central region. Overall the galaxy appears to be fairly smooth in structure. There are subtle color variations within the galaxy. The central region appears yellowish, potentially indicating an older stellar population. A slightly redder hue is noticeable towards one side, suggesting a possible region of on-going, albeit limited, star formation. The morphology suggests the possibility of a galaxy merger occurring, displaying signs of tidal disruption or interaction with another galaxy. There are no clear spiral arm structures visible.
