The galaxy presents a notable disc-like structure, although not perfectly edge-on. There is a noticeable bulge component, appearing somewhat smooth and concentrated towards the center. The disc exhibits some features and potential spiral arm segments, but they are not highly defined or tightly wound. Evidence suggests the galaxy is likely undergoing some form of interaction or disturbance. Possible signs of minor tidal distortions or merging activity can be seen in the asymmetry of the galaxy's shape. Overall, the galaxy appears to be transitioning from a relatively smooth form to a disc-dominated system with ongoing or recent interaction, exhibiting characteristics consistent with a spiral or disturbed galaxy.
