The galaxy presents as a spiral galaxy, with a disk structure that is not quite edge-on. There is evidence of spiral arm structure emanating from the central bulge. The arms are somewhat loosely wound and exhibit a patchy distribution of star-forming regions, implied by their slightly irregular color.

The central bulge appears moderately sized, exhibiting a yellowish hue suggesting a population of older stars. A weak bar structure might be present within the central region.

There is no apparent major ongoing merger event, though a minor interaction cannot be ruled out due to some visible disturbances within the disk.
