The galaxy presents as a spiral type, with a central bulge that is moderately prominent and slightly elongated. The spiral arms are loosely wound and somewhat flocculent, indicating ongoing star formation. These spiral arms appear asymmetrical. There is evidence of an interaction or minor disturbance within the galaxy's structure, potentially caused by an ongoing or recent merger event. This interaction contributes to a somewhat disrupted morphology in the outer regions of the disk. The galaxy lacks a distinct bar structure and the galactic disk is observed face-on.
