The observed galaxy appears as a relatively small, disk-shaped system viewed nearly edge-on from our line of sight. A prominent central bulge dominates the structure. The bulge appears smooth and exhibits a yellowish-white color, potentially indicating an older stellar population with less active star formation.

The galactic disk, while narrow due to the viewing angle, exhibits a diffuse and somewhat irregular morphology. There is little evidence of distinct spiral arm structure. The disk appears bluer than the bulge, suggesting the presence of younger, hotter stars and ongoing star formation. The extremities of the disk fade into the background sky, making it difficult to precisely ascertain its full extent.

No signs of major mergers or significant tidal disturbances are evident. However, some subtle irregularities in the disk's morphology could suggest minor interactions or internal processes affecting the galaxy's structure.
