The galaxy presents as a largely featureless elliptical or lenticular object, with a high degree of central concentration. Its light is dominated by older stellar populations, giving it a reddish-yellow hue. There is little evidence of spiral arms or active star formation regions within the visible wavelengths. The galaxy appears to be relatively isolated, with no obvious tidal disturbances or nearby companion galaxies that would suggest recent merger activity. It is more or less uniformly distributed, with a very mild amount of ellipticity.
