The galaxy presents a clear spiral structure, observable despite its distance. The arms are well-defined and appear to be primarily composed of Population I stars and ionized gas, indicated by their bluish hue. Dust lanes are also likely present. The galaxy appears to be dominated by a disk component and exhibits a moderate central bulge that transitions smoothly into the disk. The bulge presents a yellowish-white appearance, suggesting an older stellar population. A weak bar structure may be present, though the resolution makes it difficult to definitively confirm. The spiral arms appear to have a medium winding, indicating an intermediate type of spiral galaxy. There are two main arms, each with its own distinct morphology. There is no obvious sign of any ongoing major mergers, though some minor disturbances can not be ruled out at this resolution.