The galaxy appears to be a spiral galaxy viewed edge-on or at a very high inclination. A prominent central bulge is visible, exhibiting a bright and concentrated luminosity. The disk component appears relatively thin and elongated, with some indications of dust lanes. The overall color distribution suggests a mix of stellar populations, with a hint of bluer regions, possibly indicating areas of recent star formation, alongside generally redder regions indicating the presence of older stars. There are potential disturbances present in the disk, suggesting possible tidal interactions, but nothing that indicates a major merger. 
