The observed galaxy presents as a spiral galaxy, exhibiting a disk-like structure that is not perfectly face-on, but slightly inclined with respect to the observer's line of sight.

The galactic nucleus appears as a bright, concentrated central bulge, potentially harboring a supermassive black hole. The bulge exhibits a moderate size relative to the overall galactic structure.

Extending outwards from the nucleus are discernible spiral arms. The arms are relatively tightly wound. Within these spiral arms, there is a mottled texture suggesting active star formation regions. The star formation activity appears to be relatively low overall.

The galaxy has a yellow-orange color, suggesting the presence of older stellar populations throughout the galactic disk. This indicates the galaxy is relatively evolved. No signs of major disturbances are visible.
