The galaxy presents as a spiral with a moderate inclination relative to our line of sight. Prominent spiral arms are visible, exhibiting a tightly wound morphology. The central bulge is a noticeable component but does not dominate the overall structure, indicating a classification leaning towards a later-type spiral. There is a potential bar-like feature across the center of the bulge, although the data resolution makes that feature difficult to resolve. The disk shows a complex structure with regions of both active star formation, as suggested by the blue tinges, and older stellar populations. The structure of the galaxy is not disturbed by any merging.