The galaxy exhibits a discernible spiral structure. Multiple spiral arms are observed, displaying a relatively open morphology. The arms show clumpy regions suggestive of active star formation. The galaxy displays a central bulge, possibly containing a supermassive black hole. The bulge does not appear overly prominent in relation to the disk. A bar-like feature is present and oriented roughly horizontally, with what appears to be a slight bend. The disk is the dominant feature, and is not observed to be edge-on, but rather at a relatively high angle. The overall color is indicative of a mix of stellar populations, with some regions appearing more blue, possibly associated with younger, hotter stars.
