The galaxy presents as an elliptical morphology. It appears largely smooth and featureless, with a concentrated central bulge. The color index suggests a population of older stars, likely dominated by redder wavelengths, with very little evidence of recent star formation. Its overall symmetrical shape indicates it is unlikely to be undergoing any major merger activity, with some potential minor tidal disturbances or distortions in the outer regions. The galaxy exhibits an intermediate degree of roundness.
