The galaxy presents as a centrally concentrated object with an overall elliptical morphology, exhibiting a smooth, diffuse light distribution.  The central region appears brighter and more yellow in color, potentially indicating a higher density of older stellar populations.  The outer regions of the galaxy show a gradual decrease in surface brightness.  There are no readily apparent spiral arms or dust lanes.  The galaxy's shape is somewhere between round and elongated.  There is no indication of major disturbances to the morphology, suggesting it is not currently undergoing a major merger, though minor interactions cannot be ruled out at this resolution.
