The galaxy presents as a predominantly elliptical morphology. The light distribution appears smooth and concentrated towards the center, suggesting a relatively old stellar population. A hint of a faint disk component is present. The galaxy appears to be fairly massive, with a high likelihood that it is not currently experiencing significant star formation. There are minor signs of past or ongoing merger activity but the galaxy seems to be mostly undisturbed. The overall color of the galaxy is yellowish indicating an absence of extremely young, massive stars. The galaxy’s shape is generally round.
