The galaxy presents a centrally concentrated, generally smooth morphology, suggesting an elliptical or lenticular classification. The central region exhibits a significantly higher luminosity than the surrounding area, indicating a dense concentration of stars. The radial light profile appears to gradually decrease outwards from the center. There is a slight elongation, but the galaxy appears generally round. No distinct spiral arm features or prominent dust lanes are visible. The color is generally redder than the surrounding space. There does not appear to be any evidence of major disturbances or ongoing mergers.
