This galaxy appears to be a spiral galaxy with a prominent disk structure. The spiral arms are tightly wound around a central bulge, which is relatively small. The galaxy appears blue in color, suggesting a population of young, hot stars within the spiral arms. There seems to be a weak bar-like feature running through the center of the galaxy. The disk is not perfectly uniform, exhibiting some patchy regions. This galaxy does not appear to be undergoing a major merger, though minor disturbances cannot be ruled out.
