The galaxy exhibits a prominent disk structure with a visible bulge. The spiral arms appear to be well-defined, with a medium winding pattern, tracing from the central region outwards. The overall color suggests a mix of stellar populations, with bluer regions indicating more recent star formation in the spiral arms and a yellower central bulge associated with an older stellar population. There may be some evidence of a bar structure across the central region. The disk appears to be slightly inclined relative to our line of sight, allowing us to observe some three-dimensional structure. Some areas within the galaxy exhibit minor disturbance to their spiral structure, possibly as a result of a past or ongoing minor merger.
