The galaxy presents a distinct, well-defined spiral structure. The spiral arms are prominent and exhibit a relatively loose winding pattern. Two primary arms are clearly visible, extending from the central region of the galaxy. The disk component of the galaxy appears dominant, with a relatively small bulge. There appears to be an elongated bar-like structure. The colour distribution suggests some active star formation is occurring within the spiral arms. There are no readily apparent signs of major interactions or disturbances, although minor asymmetries cannot be ruled out based on this image alone. Overall, the galaxy appears to be a typical spiral galaxy with ongoing star formation activity within its spiral arms.
