The galaxy presents as a spiral galaxy. Its disk is visible but appears moderately inclined relative to our line of sight. There's a suggestion of spiral arm structure, although the resolution is not sufficient to delineate them clearly. The arms appear somewhat flocculent. The central bulge appears relatively small, with a small central concentration of light. There is no obvious bar structure present. There is some evidence of active star formation, visible as faint blueish regions along the spiral arms. It appears that the galaxy may be in the process of undergoing a merger event.
