The galaxy presents as a flattened, disk-like structure oriented approximately edge-on to our line of sight. There is a noticeable central bulge, appearing brighter and more concentrated than the surrounding disk. The bulge exhibits a yellowish-white hue, possibly indicating an older stellar population. 

The disk component appears relatively smooth, with no immediately obvious signs of distinct spiral arms. The disk's color appears somewhat bluer than the bulge, suggesting the presence of some younger stars. The galaxy has no major distortions in its overall shape and appears undisturbed.
