The galaxy appears as a flattened, disk-shaped structure, presented nearly edge-on relative to our line of sight. A prominent central bulge dominates the core, exhibiting a yellowish-orange hue. The disk component displays a bluer color than the bulge. The dust lane is not clearly visible but can be inferred from the light attenuation across the midplane of the disk, indicating the presence of obscuring material. There is little sign of spiral arms or prominent star-forming regions in the disk, which suggests that star formation may be relatively quiescent. Overall the galaxy exhibits a regular shape, showing no obvious signs of major disturbances or ongoing mergers. The relative uniformity and apparent lack of active star formation points towards a well-evolved system.
