The galaxy presents as a disk galaxy viewed at a moderate inclination. It exhibits a relatively smooth morphology, indicating a lack of strong spiral arm structures or significant star-forming regions that would disrupt the overall smoothness. There is a slight hint of a bulge component. It appears that the galaxy is not strongly involved in any major merging events, although there might be some minor gravitational disturbances, indicated by the presence of some faint tidal features or asymmetries in the outer regions of the disk. The overall shape is somewhat intermediate between round and elliptical, leaning towards a more rounded appearance. The light distribution suggests a mature stellar population.
