The galaxy presents a clear spiral structure, appearing as a relatively well-defined disk with prominent spiral arms. It exhibits a moderate bulge component, neither overly dominant nor negligible. The spiral arms are primarily wound with medium tightness. There is evidence of two main spiral arms. The disk is not perfectly edge-on; it is slightly tilted. There is no significant bar structure visible in this galaxy. The galaxy exhibits some disturbance, but does not appear to be undergoing a major merger. Overall, it seems to be a fairly evolved spiral galaxy with signs of ongoing star formation.
