The galaxy presents as a spiral, viewed at an oblique angle, indicating a disk morphology. The spiral arms are loosely wound and trace a clear two-armed structure. A central bulge is discernible, but not dominant, exhibiting an intermediate size. The presence of a bar structure is noted, though the strength of the bar appears moderate to weak. The overall appearance is typical of late-type spiral galaxies. There are no immediately obvious signs of a major merger event, though subtle disturbances or minor interactions cannot be entirely ruled out from the image alone.
