The galaxy presents as a flattened, disk-shaped structure, consistent with a spiral or lenticular morphology viewed nearly edge-on. A central bulge region exhibits a brighter, more concentrated luminosity, appearing yellowish-white in color. The disk extends outwards from the bulge, showing a gradual fading towards the edges. A slight warp can be discerned along the disk, giving it a non-uniform appearance along its major axis. The disk appears mottled with diffuse blueish hues, suggestive of the presence of younger stellar populations and ongoing star formation within the spiral arms. The galaxy lacks any signs of a strong bar structure. Overall, the galaxy's smooth light distribution indicates that it is largely undisturbed, and unlikely undergoing any major merging events.
