This galaxy presents a distinct spiral morphology. The arms are tightly wound, and the disk is viewed at an angle that is not quite face-on. A central bulge is visible, though it appears relatively small compared to the disk. The color of the disk is predominantly blueish, suggesting active star formation, while the bulge is more yellowish, indicating an older stellar population. There is a noticeable degree of patchiness in the spiral arms, which could be due to the presence of dust lanes or regions of intense star formation. There are no signs of a strong bar structure. The galaxy does not exhibit any obvious signs of a major merger or strong tidal disturbances, though the presence of subtle asymmetries cannot be ruled out without further investigation.
