The galaxy exhibits a distinct spiral structure, with arms emanating from a central bulge. The spiral arms appear tightly wound in some regions and more loosely wound in others. Patches of enhanced star formation are visible within the spiral arms, indicated by slightly brighter areas with a bluer hue.

The galaxy appears to be inclined relative to our line of sight, presenting an elliptical shape. The central bulge displays a yellowish color, suggesting an older stellar population. Overall, the galaxy appears to be in a relatively quiescent state, with no obvious signs of major mergers or active galactic nuclei activity. The luminosity profile suggests a relatively low Sersic index, typical of spiral galaxies.
