The galaxy presents as an edge-on disk galaxy, exhibiting a prominent dust lane bisecting its central bulge. The disk shows a distinct blueish hue, particularly at the outer edges, indicative of ongoing star formation. The central bulge appears yellowish-orange, suggesting an older stellar population. The dust lane is dark and relatively uniform, obscuring the light from stars behind it. No signs of a major merger or significant tidal disturbances are apparent in the visible structure. The disk appears thin and elongated. There may be a hint of a boxy bulge feature, though the edge-on view makes it difficult to confirm. Overall, the galaxy appears as a relatively undisturbed spiral galaxy observed at an inclination of approximately 90 degrees to our line of sight.
