The galaxy presents a generally smooth, elliptical morphology, with a highly concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. There is a subtle color gradient, with the central region appearing bluer than the outer regions, suggesting a modest degree of recent star formation, although overall, the star formation rate appears to be relatively low. The galaxy exhibits a high degree of roundness, with minimal elongation or distortion, and no apparent signs of ongoing or recent major mergers or tidal disturbances, although minor interactions cannot be ruled out.
