The galaxy exhibits a disk morphology with prominent spiral arm structures. These arms appear to be grand-design, tightly wound from the center. The central bulge is moderately sized and quite bright. There may be a faint bar structure. Evidence of active star formation is suggested by the blue hue present throughout the spiral arms, intermixed with some reddish regions that could signal older stellar populations. There is some minor disturbance in the structure that is noticeable, but not overly dominant. The galaxy's overall color profile suggests a spiral galaxy.
