The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. The overall color is indicative of an older stellar population, exhibiting a yellowish hue. There is a subtle flattening of the galaxy along one axis, suggesting some degree of ellipticity. No distinct spiral arms or dust lanes are apparent. The galaxy appears relatively undisturbed, without any obvious signs of recent merger activity, such as tidal tails or distorted morphology. The central region is brighter and more concentrated than the outer regions.
