The galaxy appears as a highly inclined, likely disk-shaped system. The central bulge is prominent, exhibiting a smooth, concentrated appearance with a yellowish-orange hue, suggesting an older stellar population. The disk component is significantly fainter and bluer than the bulge, consistent with the presence of younger stars and ongoing star formation. The galaxy seems relatively undisturbed, with no obvious signs of major mergers or tidal interactions. However, there is a subtle asymmetry to the disk, perhaps indicating a minor gravitational disturbance. Overall, the galaxy presents characteristics of a relatively massive, star-forming spiral galaxy observed at a considerable distance, with the disk seen nearly edge-on.
