The galaxy appears as a largely featureless elliptical or lenticular system. It has a concentrated central bulge that diminishes in luminosity outwards, with a smooth transition. The galaxy is generally round in appearance, with no obvious deviations from this shape. There is no visible structure in the form of spiral arms or a distinct disk component. There is no noticeable dust lane or bar structure. The galaxy appears to be an isolated system, as there are no signs of tidal distortions or ongoing merger activity. The color profile suggests a population of older stars, as indicated by the galaxy's yellowish to reddish hue.
