The galaxy presents as a spiral type with a prominent disk structure. The disk exhibits clear spiral arm features, estimated to be a two-armed spiral galaxy, characterized by a loosely wound morphology. A central bulge is visible, exhibiting a moderate size relative to the disk, and a faint bar feature appears to be present in the central region. Evidence suggests a relatively low rate of recent merging activity, although some minor disturbances may be present. The galaxy displays a moderate amount of star formation, indicated by the presence of blue light associated with the spiral arms. The galaxy is neither perfectly edge-on nor face-on, but at a non-extreme angle.
