The galaxy presents as a flattened, disk-like structure seen nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component appears relatively smooth, with a bluer tint compared to the central bulge. The galaxy displays a noticeable dust lane, likely composed of interstellar dust and gas, bisecting the galaxy along its equatorial plane. There are no apparent signs of ongoing major mergers. The outer regions of the disk appear diffuse, with some irregularities.
