This galaxy presents as a flattened, disk-like structure seen nearly edge-on. The central region appears brighter and more concentrated, exhibiting a yellowish hue indicative of an older stellar population. Moving outwards from the core, the galaxy's light becomes fainter, with a more diffuse, bluish color suggesting the presence of younger, hotter stars. There is a subtle hint of dust lanes or obscuring material along the plane of the disk, further supporting an edge-on perspective. The overall shape is elongated, and there's no immediately obvious sign of major interactions or mergers. The morphology is generally smooth, with only subtle features suggestive of ongoing star formation or minor disturbances.
