The galaxy exhibits a generally diffuse morphology. The light distribution appears asymmetrical with areas of bright, diffuse regions interspersed with darker patches. A slight spiral structure may be present, but its form is difficult to ascertain due to the galaxy's overall irregular appearance and the presence of what may be dust lanes. There may be merging or tidal features that are disturbing the galaxy's morphology. There appears to be multiple merging events occurring, causing the disturbances. There is a strong central bulge, with distinct areas of disturbances within it. 