The observed galaxy presents as an edge-on spiral, characterized by a prominent, extended disk. A central bulge is evident, exhibiting a rounded morphology. The disk structure appears largely undisturbed with no indications of major mergers or tidal interactions. The galaxy's color profile displays a gradient, with the central bulge exhibiting a more yellowish hue, suggesting an older stellar population. The outer regions of the disk show a bluer tint, which may suggest recent star formation. The disk exhibits a smooth, rather than patchy, distribution of light. There is no obvious dust lane visible, but the lack of a sharply defined edge suggests a smooth transition in stellar density from the disk into the surrounding halo.
