The galaxy presents as a flattened, disk-like structure viewed nearly edge-on. There's a prominent central bulge that appears somewhat elongated. The bulge exhibits a yellowish hue, potentially indicative of an older stellar population. The disk itself appears relatively smooth, lacking the distinct spiral arm structures associated with grand-design spirals, although there are some faint irregularities along the edges. A dark dust lane is not clearly visible, however the galaxy disk is very thin. The galaxy's color is bluer toward the outer regions of the disk, suggesting the presence of younger, hotter stars, indicating regions of active star formation. There are no signs of significant tidal disturbances or ongoing mergers.
