The galaxy exhibits a prominent spiral structure, characterized by two well-defined spiral arms that emanate from a central bulge region. The winding of these arms appears relatively loose. The bulge itself presents a moderate size relative to the overall disk. The disk is oriented face-on, allowing for a clear view of its spiral morphology. There is no indication of a strong central bar feature. The overall morphology suggests a classification as a spiral galaxy. Indications of merging or major tidal disturbances are apparent within the galactic structure, which may be related to a non-relaxed morphology and irregular arm structures. The red shift value indicates that the galaxy is relatively far away.
