The galaxy presents as a spiral type, exhibiting a generally flattened disk structure. Two well-defined spiral arms are distinctly visible, showing a loosely wound morphology. The central bulge appears relatively small and not especially prominent, with a slight bar structure extending through its center. Star formation is apparent throughout the galaxy, with numerous regions of blue indicating younger, hotter stars populating the spiral arms. The overall shape suggests a fairly regular spiral structure, though some minor distortions or irregularities may be present, indicating a possibility of past minor interactions. There are no signs of any major mergers or other mergers occurring. The galaxy is not edge-on, showing clear disk features with no signs of an obscured midplane.
