The galaxy exhibits a clear spiral structure. Two arms emanate from the central bulge region. These arms are tightly wound, implying that the galaxy is relatively old and has experienced considerable differential rotation.

The central bulge appears moderately prominent, with a yellowish hue. It suggests an older stellar population, perhaps a significant concentration of Population II stars. The spiral arms exhibit a bluer color, suggesting a younger stellar population and ongoing star formation.

There is evidence of a bar structure running through the galactic center. This feature may contribute to the channeling of gas towards the central regions, potentially fueling star formation activity and the supermassive black hole.

The disk of the galaxy is not perfectly smooth. This could be due to some minor gravitational disturbances.
