The observed galaxy presents as an edge-on spiral system. A prominent central bulge dominates the morphology, exhibiting a yellowish hue indicative of an older stellar population. The disk appears thin and elongated, with the dust lane bisecting the galaxy and obscuring a portion of the light from behind. The disk displays a bluer color, which may indicate recent or ongoing star formation. There is a small indication of a spiral arm on the upper right of the galaxy. The light distribution suggests it may be a galaxy with an estimated stellar mass around 10^11 solar masses and relatively low star formation activity.
