The galaxy appears as a flattened, disk-shaped structure with an elongated morphology. The central region exhibits a bright, concentrated bulge. The disk component displays a smooth texture, with hints of spiral arm structures, however, they appear diffuse. There seems to be ongoing star formation, as suggested by the slightly bluish tint observed in the disk and around the bulge. There are slight disturbances visible, but it is unclear if they are a result of any tidal interactions with a neighbor. No bar is visible in the central region.