The observed galaxy presents a clear disk morphology, viewed at an oblique angle, indicating it is not precisely face-on nor edge-on. A distinct central bulge is apparent, exhibiting a moderate size relative to the overall disk. Evidence of spiral arm structure is visible within the disk.

The galactic bar appears to be a moderate component of the galactic structure.

There is no obvious signs of major disturbances and no indications of merger activity and it does not appear to be undergoing any significant interactions with companion galaxies.
