The galaxy presents as an edge-on spiral, exhibiting a notably elongated morphology. A prominent central bulge is apparent, with a rounded shape. The disk component is visible, displaying a relatively smooth texture. Faint, diffuse dust lanes may be present. There is no clear evidence of strong spiral arm structure. The galaxy shows no signs of a major ongoing merger event, though some minor disturbances cannot be ruled out. The overall color profile appears to be typical of a galaxy with moderate star formation, with a generally redder appearance. 
