The galaxy presents a morphology consistent with a spiral structure. The spiral arms are readily apparent, exhibiting a relatively open winding pattern. A prominent central bulge is visible, appearing moderately sized compared to the overall galactic disk. The bulge appears to be spheroidal in shape. A bar-like structure is visible traversing the central region of the galaxy. There appears to be some distortion of its morphology indicating a possible interaction or merger in its recent past. The disk component is viewed at an oblique angle, not precisely edge-on.
