The galaxy presents as a generally smooth and elliptical-like structure. The central region exhibits a significantly brighter and more concentrated luminosity, potentially indicating the presence of a substantial galactic nucleus. There is a visible radial gradient in the light intensity, with brightness decreasing smoothly from the core to the outer regions. The galaxy's color appears to be primarily yellowish, shifting towards redder hues further from the center. The morphology appears relatively undisturbed, and there are no obvious signs of ongoing major merger events. There is a slight elongation in the structure indicating that it is not perfectly round, perhaps closer to in between round and cigar shaped. The overall appearance suggests that this is a relatively massive galaxy with a low rate of star formation.
