The galaxy presents a clear spiral structure, with two prominent arms emanating from a central bulge. These arms appear loosely wound, suggesting differential rotation and potentially ongoing star formation within. The central bulge has a moderate size relative to the disk, displaying a concentrated luminosity that may indicate a significant population of older stars. A weak bar-like structure appears to extend through the central region, influencing the morphology of the inner spiral arms. The disk is viewed at a slight inclination, providing a partial view of its overall structure. There are no immediately obvious signs of major merging activity, although some minor disturbances cannot be ruled out based on this image alone.
