This galaxy presents as an edge-on spiral, exhibiting a flattened disk structure. A prominent central bulge is visible, appearing rounded and concentrated. The dust lane bisecting the galaxy's disk is clearly defined and relatively uniform, obscuring a portion of the starlight from the far side of the disk. The galaxy displays a yellowish-orange hue throughout its structure, suggesting an older stellar population with diminished ongoing star formation. There is no evidence of significant tidal features or major disturbances, indicating it has likely undergone no recent major merging events. Faint hints of spiral arm structure are subtly visible as they emerge from the bulge, and become wider across the extent of the disk. 
