The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a slight elongation, but the overall shape is tending towards round. The galaxy's light profile appears diffuse, lacking strong central concentration. The galaxy exhibits a color gradient, shifting from bluer hues in the central region to redder tones in the outer parts of the galactic halo. Based on these characteristics, it is possibly a quiescent, massive galaxy with a low rate of star formation. There is evidence of potential merging activity to the galaxy.
