The galaxy presents as a centrally concentrated object with a relatively smooth morphology. It is generally elliptical in shape. The light distribution suggests it may be a lenticular galaxy. There is a slight color gradient, with the core appearing somewhat redder than the outer regions. There is no evidence of significant disk features or spiral arms. There appears to be no signs of major disturbances in the galaxy's structure, such as tidal tails or merging companions. Overall, the galaxy appears to be a relatively undisturbed system with an evolved stellar population.
