The galaxy exhibits a disturbed morphology, suggesting potential tidal interactions or a recent merger event. There is a prominent central bulge with a relatively smooth texture. Faint diffuse arms extending from the central region are visible, with some clumpy regions indicating areas of active star formation. Overall the structure seems to show no clear disk morphology, appearing more amorphous. A large amount of artifact contamination exists, obscuring a clear picture of this galaxy. The red component suggests older stellar populations or dust presence, while the green and blue might indicate regions with younger stars.
