The galaxy presents as a relatively smooth, elliptical structure. Its light is fairly concentrated, with a brighter central region fading into a diffuse outer halo. There is little to no evidence of spiral arms or a distinct disk. The galaxy appears approximately circular. The color is generally a pale blue, potentially indicating a moderate amount of star formation activity. There are no obvious signs of tidal tails or distortions, suggesting it is not currently undergoing a major merger event, although some minor disturbances cannot be ruled out. 
