The galaxy exhibits a flattened, disk-like morphology, viewed edge-on from our vantage point. A prominent central bulge is evident, appearing brighter and more concentrated than the surrounding disk. The bulge displays a yellowish-white hue, suggesting an older stellar population. A distinct, dark dust lane bisects the galaxy's disk, obscuring light from the stars and gas behind it. This dust lane appears reddish in color. Faint extensions or tidal features are not immediately apparent, suggesting the galaxy is relatively undisturbed. There are no obvious signs of recent major merger activity. The galaxy exhibits a relatively smooth profile, but some features are observed.
