This galaxy exhibits a strong spiral structure, characterized by prominent, well-defined arms. These arms appear to be tightly wound, forming a discernible pattern as they emanate from the central region. The central bulge is relatively small, suggesting a late-type spiral galaxy. There is evidence of a bar-like feature extending across the center of the galaxy, with a moderate prominence. In addition, there are signs of ongoing merger activity or significant gravitational disturbances present in the surrounding areas of the galaxy, with some irregularities visible in the structure. Overall, the galaxy presents a complex and dynamic morphology, consistent with the ongoing processes of galaxy evolution.
