The galaxy presents as an edge-on spiral, exhibiting a clearly defined, elongated disk structure. A prominent dust lane bisects the galaxy horizontally, obscuring the central bulge region. The bulge appears relatively small and rounded, with a smooth texture, showing little to no distinct substructure. There is a clear distinction between the disk and the bulge. The galaxy does not appear to be undergoing any major mergers or significant tidal interactions. The disk shows hints of spiral arm structure, though obscured by the dust lane. The disk is relatively smooth, showing a general decrease in brightness as it expands outwards from the central bulge.
