The galaxy presents an intermediate morphology, possibly transitioning between a smooth elliptical form and a more disk-like structure. The central region exhibits a higher concentration of light, suggesting a bulge component. There is evidence of features disrupting the smoothness. The presence of some blue color may indicate recent star formation within the galaxy. Faint tidal features are present. These observations suggest the possibility of a recent or ongoing minor merger event. The red light is most likely from the presence of older stars or dust. The merging fraction is low, and the merger disturbance is minor.
