This galaxy exhibits a morphology consistent with a spiral galaxy, although its disk is not perfectly face-on, showing a slight inclination relative to our line of sight. The galaxy displays a notable central bulge with a yellowish-orange hue, suggesting an older stellar population. Fainter spiral arms extend outwards from the central bulge region. These arms appear somewhat loosely wound and patchy, displaying some blueish tinges indicative of younger, hotter stars and regions of active star formation. There is no obvious presence of a strong bar structure. There are slight signs of gravitational disturbance or tidal features suggesting possible interaction with another galaxy, however they appear minor. There is no significant dust lane visible, and the disk appears relatively smooth.
