The galaxy presents as a spiral, characterized by distinct arms emanating from a central bulge. The spiral arms display a well-defined structure with a predominantly two-arm morphology. The winding of these arms appears relatively tight in some regions and of medium pitch in others, suggesting variations in rotational velocity or density waves across the galactic disk.

The central bulge exhibits a moderate size relative to the disk, with a yellowish hue, indicating an older stellar population dominating the core. The spiral arms show bluer tones, implying ongoing star formation regions. Faint hints of dust lanes are observed, particularly along the inner edges of the spiral arms, suggesting the presence of interstellar material. The overall shape of the galaxy appears relatively undisturbed.
