The galaxy presents a generally smooth morphology, with a slight preference for an elliptical shape over a fully circular one. It shows some features that might indicate slight disturbances or asymmetries in its structure. There's no single, well-defined nucleus, but rather a more diffuse central region. The galaxy exhibits a color gradient, appearing bluer towards its center and becoming redder and slightly fainter in the outer regions. The color suggests the presence of some ongoing star formation, localized toward the center. There may be weak evidence of a disk.
