The galaxy appears to be a spiral galaxy viewed edge-on. Its morphology suggests a significant disk component. The central bulge seems prominent and has a rounded appearance. There is no clear indication of a boxy bulge. The galaxy shows no obvious signs of recent major mergers or strong tidal disturbances, although a minor perturbation can't be ruled out. The color profile indicates a strong presence of older stellar populations, resulting in a reddish hue. Given its size and spectral properties, it's a galaxy with a significant mass, currently undergoing moderate levels of star formation.
