The galaxy presents a disk-like structure with an apparent edge-on orientation relative to the observer's line of sight. Faint spiral arm features are visible along the primary axis of the disk. The central bulge appears prominent, although not entirely dominant, exhibiting a moderate size relative to the overall galactic structure. The bulge has a smooth texture, indicating a lack of significant star forming regions. 

A slight warping is observed within the galactic disk, suggesting potential gravitational interaction or minor disturbance. Overall, the galaxy does not exhibit signs of major ongoing mergers or significant tidal distortions, although minor disturbances cannot be ruled out based on the structure of the disk. No distinct bar-like structure is discernible within the central bulge. The galaxy appears to be relatively isolated.
