The observed galaxy presents as a spiral galaxy viewed nearly edge-on. A prominent dust lane is visible, bisecting the galaxy's disk and obscuring a significant portion of the stellar light, particularly near the central region. The bulge appears flattened, almost lenticular in nature, with a slight asymmetry. The disk displays subtle color variations, with bluer hues potentially indicating regions of active star formation. No significant signs of a major ongoing merger or tidal disturbances are apparent, however a very faint asymmetrical structure may be present. The overall structure suggests a galaxy that is relatively undisturbed and evolving in isolation.
