This galaxy presents as an edge-on spiral, exhibiting a prominent central bulge. The bulge displays a yellowish hue, indicating an older stellar population. The disk appears relatively smooth with minimal discernible spiral arm structure. The galaxy appears to be quite large with an estimated physical radius over 12 kpc. The disk of the galaxy appears very thin, without substantial substructure in the images. There is no evidence of a major merger, or any nearby companions.
