The galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology with a notable central bulge. The bulge appears relatively bright and concentrated. Dust lanes are visible, though somewhat indistinct, along the galactic plane, contributing to a mottled appearance. There is an apparent lack of resolved star-forming regions or prominent spiral arm structure, with a relatively smooth overall luminosity gradient from the bulge outwards along the disk. The ellipticity of the galaxy is significant, indicating a highly inclined viewing angle relative to the plane of the disk. No signs of major mergers were immediately observed.
