The galaxy presents as a spiral type, exhibiting a notable disk structure. The central bulge region appears relatively small and somewhat indistinct. Spiral arms are visible, and appear to be present around a central bar structure. The arms are not tightly wound, suggesting a later type spiral morphology.  Evidence of ongoing star formation is indicated by the bluer coloration, particularly within the spiral arms.  The overall shape suggests a potentially ongoing or recent merger event, showing some morphological disturbance. The disk is oriented at an angle to our line of sight, but not completely edge-on.
