The galaxy presents as a largely smooth, centrally concentrated object with a slight ellipticity. There is minimal evidence of spiral arm structure or distinct features. The overall color is redder, concentrated towards the core, indicating a relatively older stellar population. There is some evidence of a disk, however it appears small and featureless. The high degree of central concentration and lack of prominent disk features suggests that this is likely an elliptical galaxy, though the small disk cannot be ruled out, nor can the features be ruled out with the image quality. No obvious signs of recent merger activity are apparent.
