The galaxy presents a spiral morphology, albeit somewhat disturbed. The central bulge is a prominent feature, appearing relatively large and contributing significantly to the overall luminosity of the system. Faint spiral arm structures are discernible, displaying a moderate winding and appear relatively tightly wound closer to the central bulge. There appears to be at least two or three distinct arms.  Evidence suggests ongoing star formation activity in the disk regions, as subtle color variations within the arms suggest regions of potentially higher temperatures. The galaxy's morphology suggests it may be undergoing some minor gravitational disturbance from a past or ongoing merger event.
