The galaxy presents as a predominantly edge-on spiral. A flattened disk structure is clearly visible, with a central bulge. The bulge appears to be largely rounded. There is no evidence of a boxy morphology to the bulge. 

Within the disk, there's an absence of significant, well-defined spiral arm structures. The disk exhibits a relatively smooth appearance. There appears to be a slight asymmetry in the dust lane, hinting at a mild warp or disturbance. 

There is no discernible evidence of a major merger or significant tidal disturbances. A potential minor disturbance cannot be ruled out.
