The galaxy presents an edge-on disk morphology. A prominent, centrally located bulge dominates the overall structure. The bulge exhibits a smooth, rounded appearance. The disk appears thin and elongated, with a relatively uniform color gradient extending outwards from the central bulge. The color distribution suggests a decreasing concentration of older stellar populations towards the outer regions. The galaxy's disk exhibits an apparent dust lane along the mid-plane, indicative of gas and dust obscuration. There are hints of possible disturbances in the disk at one end of the galaxy, evidenced by a color shift. The galaxy is otherwise relatively undisturbed.
