The galaxy presents as an elongated, disk-shaped structure viewed edge-on. A prominent central bulge is visible, exhibiting a relatively smooth, rounded morphology with a yellowish hue. The disk component appears thin and extended, with a slight hint of dust lane obscuration along the equatorial plane. The overall color gradient suggests older stellar populations concentrated in the bulge, while younger, bluer stars may be present within the disk. There are no clear signs of significant tidal disturbances or ongoing merger activity, although subtle asymmetries in the disk structure cannot be ruled out given the resolution. The galaxy appears relatively isolated within its immediate environment.
