The galaxy presents as a flattened, disk-like structure, oriented nearly edge-on from our line of sight. A prominent central bulge exhibits a yellowish-white hue, suggesting an older stellar population dominating this region. The disk component displays a bluish tint, indicating the presence of younger, hotter stars, potentially within spiral arms. The disk appears slightly warped or disturbed, deviating from a perfectly flat plane.  Faint dust lanes are possibly visible within the disk, silhouetted against the starlight. There is a suggestion of ongoing or recent star formation, especially in the outer regions of the disk.  The overall structure suggests a possible recent interaction or merger.
