The galaxy presents as a face-on or nearly face-on spiral, exhibiting prominent spiral arm structures. These arms are well-defined, though their exact number is difficult to discern, and they appear to wind relatively tightly around the central bulge. The bulge itself is of moderate size, not overly dominant but clearly present. A bar structure within the central region is subtly suggested, though not overwhelmingly prominent. The overall form suggests a relatively unperturbed morphology, with no immediately obvious signs of major ongoing mergers, though minor disturbances cannot be ruled out. Star formation appears to be actively occurring within the spiral arms, as suggested by their bluer color, while the central bulge region presents a more yellow/red hue, potentially indicative of an older stellar population and diminished star formation rate.
