The galaxy presents as a fairly smooth, elliptical-like structure, though the resolution limits detailed morphological assessment. Its overall color appears to be somewhat redder, suggesting an older stellar population, consistent with a lower rate of star formation. The central region is brighter and more concentrated, with a gradual decrease in luminosity towards the outer edges of the galaxy. There is a very faint hint of some possible tidal disturbance or asymmetry on one side, but it would be hard to be conclusive. The galaxy displays a generally regular shape.
