The galaxy presents as a spiral structure with a moderate central bulge. The spiral arms are well-defined but appear tightly wound, extending from the core region outward. These arms exhibit a clumpy morphology, suggesting active star formation regions or dust lane obscuration. The galaxy lacks a strong central bar structure. While some asymmetry is observed in the outer disk, there is no obvious evidence of a major ongoing merger or significant tidal disturbance, although minor interactions cannot be ruled out. The central bulge appears relatively small compared to the overall disk size. A significant portion of the galaxy's structure is challenging to discern given the image resolution.
