The observed galaxy presents a clear spiral structure. Two distinct arms emanate from the central region and appear loosely wound. The disk exhibits a blue hue, suggesting the presence of a young stellar population within these arms. The bulge appears relatively small compared to the disk, with a more yellow-orange tint. There is evidence of a bar structure, possibly of medium strength, crossing the central region. No apparent major disturbances are present in the galactic structure, although some subtle asymmetries cannot be ruled out. There are no obvious signs of a large scale merger. The galaxy is not seen edge-on.
