This galaxy exhibits a prominent, well-defined spiral structure. Two spiral arms are clearly discernible, extending outwards from a central bulge. The arms appear relatively tightly wound, exhibiting a moderate pitch angle. The galaxy shows distinct blue hues throughout its disk, suggesting active star formation regions, particularly within the spiral arms. The central bulge is apparent, exhibiting a yellowish color, indicating a relatively older stellar population. There does not appear to be a strong central bar feature. The overall morphology suggests a relatively unperturbed, mature spiral galaxy, with no signs of major mergers or tidal disturbances although there seems to be a minor disturbance in the upper left arm.