This galaxy presents as a relatively small, edge-on spiral galaxy. Its shape is elongated and linear. There is a slight bulge in the center of the galaxy, with the light appearing brightest in this region. The disk component exhibits some degree of internal structure, with subtle variations in color and luminosity across its extent, though without defined or easily discernible dust lanes. The galactic disk is thin and flat. The overall color index suggests the presence of both older stellar populations (more red) and ongoing star formation (more blue), with the redder colors appearing more prominent towards the central bulge. The apparent smoothness of the light distribution suggests a lack of significant ongoing mergers or major disturbances. 
