The galaxy exhibits a spiral morphology, characterized by two prominent and tightly wound spiral arms. These arms extend from a central bulge, which appears moderately sized in relation to the overall galactic disk. The spiral arms display clumpy regions, suggestive of active star formation regions. The bulge appears yellowish, indicating an older stellar population. The disk is viewed close to face-on. There appears to be a possible, subtle bar structure across the central region of the galaxy. Overall, the galaxy does not exhibit signs of major interactions or mergers.
