The galaxy presents as a highly inclined, edge-on spiral or lenticular galaxy. Its overall morphology suggests a flattened disk-like structure. A prominent central bulge is observed, exhibiting a smooth, concentrated distribution of light, with a slight yellowish color that could indicate an older stellar population. The disk component appears relatively smooth, with a faint bluish tint, possibly indicating the presence of some ongoing star formation. The light is more concentrated in the central region. The galaxy lacks any immediately discernible spiral arm structure, or any evidence of tidal features or recent merger activity. There is some dust obscuration evident along the galactic plane. The general form is lenticular, and highly flattened.