The galaxy presents as a flattened, disk-like structure, viewed nearly edge-on from our vantage point. It exhibits a central bulge that appears relatively smooth and concentrated, diminishing in brightness towards the outer regions of the disk. The disk itself displays a layered structure, with varying degrees of light intensity suggesting potential spiral arm formations, although these are difficult to discern due to the edge-on orientation.

There is some indication of asymmetry within the disk, with one side appearing slightly more extended or disturbed than the other. The overall color profile appears consistent, with no stark differences in color visible across the galaxy. The texture of the disk seems smooth, without large-scale irregularities or distinct star-forming regions readily apparent. The galaxy displays a considerable degree of flatness. There does not appear to be any evidence of a large-scale merger or tidal disruption affecting the galaxy's morphology, though subtle irregularities are present.
