The galaxy presents a roughly elliptical morphology, appearing somewhat elongated. Its central region exhibits a high degree of luminosity, appearing as a smooth, bright concentration of light. Proceeding outward from the core, the light gradually diminishes with no distinct spiral arm structures. The light throughout the galaxy seems to shift from redder to bluer hues, suggesting varying stellar populations or dust content within the galaxy. There is some evidence of asymmetry, with what seems to be a slight extension. Further analysis would be required to confirm this. There do not appear to be any obvious signs of ongoing major merger activity or significant tidal disturbances. 
