The galaxy appears to be a relatively smooth, elliptical-like structure. There is no clear evidence of spiral arms or a distinct disk component. The light is centrally concentrated, with a gradual decrease in luminosity as you move outwards from the core. Color variations are subtle, with a possible slight reddening towards the center. There is no evidence of any major merger events or significant tidal disturbances affecting its overall morphology. The object's appearance suggests that it is likely a well-formed galaxy that has undergone some period of quiescence or a lack of recent major star formation activity. Its overall shape is consistently round. There are no obvious signs of distinct features or substructures within the galaxy's visible extent.
