The galaxy appears to be an elliptical type, characterized by a generally smooth and featureless morphology. The light is concentrated towards the center with a decrease in intensity gradually radiating outwards, and it displays an ovoid shape; not perfectly spherical, but not significantly elongated. Its color profile suggests an older stellar population, primarily composed of stars towards the redder end of the spectrum. There are no distinct spiral arms or visible dust lanes within the galaxy. The galaxy's core is fairly bright. No interactions or tidal disturbances are readily apparent; it appears as an isolated system.
