This galaxy presents as an edge-on spiral system, viewed from approximately 0.22 redshift. A prominent dust lane bisects the galaxy's main disk, obscuring a significant portion of the central bulge. The bulge itself appears rounded and luminous. Diffuse, fainter light emanates from the outer regions of the disk. Evidence suggests it exhibits disk-like characteristics rather than a smooth elliptical profile, indicating ongoing or recent star formation activity. There are slight signs of disturbances, but appears as a non-merging object.
