The galaxy presents as a relatively smooth, elliptical-like object. There is little to no discernible disk structure. The light distribution appears concentrated towards the center, suggesting a bulge-dominated morphology. The galaxy exhibits a color gradient, appearing more yellow-red at the core and slightly bluer towards the outer regions, which indicates older stellar populations concentrated in the center, and areas of possible star formation in outer areas. The overall shape tends toward the round, with a smooth and undisturbed appearance. There are no obvious signs of ongoing major merging activity, although a minor interaction cannot be entirely ruled out based on the available data.