The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, relatively featureless morphology. Its overall shape is nearly circular, suggesting a low degree of observed ellipticity. The light distribution is centrally concentrated, with the brightest region located at the core and a gradual decrease in luminosity towards the outer edges. The core displays a yellow to reddish hue, which indicates an older stellar population. This redder color suggests minimal ongoing star formation. The galaxy shows no obvious signs of tidal disturbances or active galactic nuclei, and does not appear to be interacting with any other nearby system.
