The observed galaxy presents as an edge-on spiral galaxy, with a prominent bulge. The bulge region exhibits a yellowish-white hue, suggestive of an older stellar population. The disk is highly inclined, obscuring any detailed spiral structure. The galaxy displays an elongated shape, consistent with an edge-on orientation. Dust lanes appear subtly within the disk, particularly near the central bulge, attenuating light and causing a mottled appearance. The outer regions of the disk fade into the background sky, exhibiting a bluer tint compared to the central bulge, which likely indicates the presence of younger, hotter stars. The overall morphology suggests a relatively evolved system with ongoing star formation in the outer regions. The lack of any tidal features indicates no recent major merger events, though minor disturbances can not be ruled out. The galaxy appears isolated within the field of view.
