The observed galaxy presents as a relatively smooth, disk-like structure, elongated along its major axis. Its morphology is most likely an elliptical galaxy or a lenticular galaxy viewed edge-on. A central bulge is apparent, exhibiting a concentrated luminosity profile. The overall color distribution indicates a dominant population of older stars within the bulge, potentially indicating a cessation or reduction in star formation activity in the central region. Fainter, bluer regions at the lower edge suggest a more recent episode of star formation, in at least a small part of the galaxy. The light is generally smooth, though very dim. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
