The galaxy exhibits a clear spiral structure with arms emanating from a slightly prominent central bulge. The spiral arms appear relatively tightly wound around the core, indicating a possible grand-design structure. The arms are somewhat flocculent, with varying degrees of brightness and distinctness. There's evidence of ongoing star formation within the arms, visible as subtle color variations, particularly towards the outer edges of the disk. The bulge is compact, contributing to the overall luminosity of the galaxy's core. The disk appears to be viewed at a moderate inclination. There are no obvious signs of a strong bar structure. Possible distortions can be noted in the spiral pattern, indicating there is an external factor influencing the galaxy's structure. No signs of major ongoing merger activity are present.
