The galaxy presents a spiral morphology viewed at a slight angle from face-on. The central bulge appears moderately sized, showing a diffuse, yellowish-white coloration. Spiral arms are discernable, exhibiting a relatively tight winding pattern as they emanate from the central region. Evidence suggests multiple arm structures, although defining a precise number is challenging due to image resolution. A subtle disctortion is suggested.

The overall colour of the spiral arms trends towards a bluer hue, implying the presence of younger stellar populations and ongoing star formation within the disk. No strong bar structure is clearly visible.

There is no obvious signs of a ongoing major merger.
