The galaxy presents as a disk-shaped system, viewed at an oblique angle. There is a discernible bulge, appearing yellowish-white, concentrated towards the galactic center, suggestive of an older stellar population. The disk itself exhibits a bluer hue, particularly at its edges, hinting at ongoing star formation in these regions. The galaxy's shape is elongated, leaning towards a cigar-like appearance. The overall structure appears relatively undisturbed, with no obvious signs of a recent major merger event. There is a slight asymmetry to the disk's light distribution.
