The galaxy exhibits a relatively compact morphology. Its overall structure appears to be largely smooth with no prominent spiral arms or disk features readily discernible in this imaging. However, the galaxy does show a slight asymmetry and a hint of tidal disturbance, perhaps indicative of a past or ongoing minor merger event. The central bulge is not sharply defined. There may be faint tidal tails or debris extending from the main body of the galaxy. The color is more weighted towards the green than the red, with the outer edges of the galaxy slightly redder than the inner portion.
