This galaxy presents as an edge-on spiral or lenticular galaxy, exhibiting a flattened disk structure. The central bulge appears relatively prominent, with a smooth, diffuse luminosity profile, suggesting an older stellar population. The disk shows faint dust lanes obscuring some of the starlight, particularly along the midplane. Star formation seems to be present within the disk, as evidenced by the slightly bluer colors and possible HII regions. The overall color gradient implies a radial distribution of stellar populations, with the bulge being redder and the outer disk being bluer. No signs of recent major mergers or significant tidal disturbances are evident. The galaxy exhibits a moderate redshift, indicating a substantial distance and therefore, an intrinsically high luminosity.