The galaxy appears to be a spiral galaxy viewed at an angle slightly inclined from face-on. It exhibits a distinct central bulge that appears moderately bright. The spiral arms are visible, though somewhat tightly wound and fragmented, suggesting a flocculent or multi-armed structure. The colouration indicates active star formation regions within the arms. There appears to be a bar feature running through the center of the galaxy. Overall morphology suggests the presence of ongoing interactions or disturbances within the galaxy, as its structure is not perfectly symmetric. There is some evidence of internal dust lanes.
