The galaxy presents as a face-on spiral with well-defined spiral arms. These arms appear to be of intermediate pitch. The spiral structure suggests two dominant arms. The central bulge is prominent and appears moderately sized in relation to the disk. There is no clear evidence of a bar structure. The galaxy exhibits no obvious signs of a major ongoing merger, although some minor disturbances may be present in the disk. Overall, it appears as a relatively undisturbed spiral galaxy. The winding of the spiral arms appears to be medium. There are two main spiral arms, as well as a third less defined arm.
