This galaxy exhibits a prominent, moderately sized central bulge. Surrounding the bulge is a disk structure displaying well-defined spiral arms. The arms are relatively tightly wound, suggesting a grand design spiral structure. The color of the arms indicates active star formation, likely with a notable presence of HII regions. Indications suggest multiple spiral arms. The disk is not perfectly symmetric; some irregularities possibly indicate minor gravitational interactions. The overall morphology suggests a classification as a spiral galaxy, potentially undergoing a minor merger or disturbance.
