The galaxy appears as a flattened, disk-shaped system, viewed nearly edge-on from our line of sight. It has a prominent central bulge, which is brighter and more yellow in color than the rest of the galaxy. The disk appears relatively smooth with a faint bluish hue, particularly at the outer edges. This suggests the presence of ongoing star formation activity, primarily concentrated in the disk. No spiral arm structure is clearly visible, and there is no evidence of any major disturbances or merging activity. The galaxy appears relatively isolated and undisturbed.
