The galaxy presents a distinct spiral morphology. High inclination of spiral arms, appear tightly wound and well-defined, originating from a central bulge. The bulge exhibits a yellowish hue, potentially indicative of an older stellar population. The spiral arms are bluer in color, suggesting ongoing star formation within. The overall structure suggests a mature spiral galaxy, potentially experiencing a moderate rate of star formation. There is some slight irregularity in the overall disk shape.
