This appears to be an edge-on spiral galaxy, exhibiting a flattened disk structure viewed almost perfectly from the side. The galaxy displays a prominent central bulge that appears reddish-orange in color. This suggests an older stellar population, potentially composed of evolved giant and supergiant stars. Fainter, bluer light is observed emanating from the disk. This suggests active star formation, potentially with populations of hotter, younger stars. There is no evidence of a bar structure. The disk has a distinct, sharp edge, indicating a relatively thin disk component. There is no evidence of a significant tidal disturbance, merger activity, or major asymmetries in the galactic morphology. Given the smoothness of the disk, it is likely that this is a relatively undisturbed galaxy with ongoing star formation. The galaxy disk is inclined at a very high angle to our line of sight.
