The galaxy exhibits a flattened, disk-like morphology, characteristic of a spiral galaxy viewed at an oblique angle to our line of sight. The central bulge appears prominent and exhibits a yellowish hue, indicative of an older stellar population. Faint spiral arm structures extend outwards from the bulge, showing a somewhat tightly wound pattern. The arms display a bluer color, suggesting ongoing star formation activity within these regions. A strong central bar is visible through the center. The overall ellipticity of the galaxy is high. There is no clear evidence of active galactic nuclei activity or a significant amount of dust obscuration.
