The galaxy presents as a flattened, elongated structure, suggestive of an edge-on disk galaxy. A prominent bulge is observed at the center, exhibiting a yellowish hue. This central region likely contains an older stellar population. The disk component appears relatively smooth, extending outwards from the bulge. There is evidence of some blue color on the far extents of the disk, indicating ongoing star formation, but this is not the main form of light emission from the disk. The galaxy lacks any strong signs of spiral arm structure or active galactic nuclei.
