The galaxy presents a disk-dominated morphology, characterized by a prominent central bulge. The bulge appears moderately sized relative to the overall galactic structure. Spiral arms are visible, exhibiting a two-armed grand design with a medium winding pattern. Evidence suggests the presence of a bar structure across the galactic center, estimated to be on the stronger side. There is no indication of any ongoing major merging events, although there is likely a minor disturbance.
