The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated brightness profile, with luminosity decreasing gradually toward the outer regions. There is a subtle color gradient, with the core appearing slightly redder than the outer halo. No distinct spiral arm structures or dust lanes are discernible, contributing to the smooth overall appearance. The galaxy appears relatively isolated, showing no clear signs of major interactions or mergers in its current state, though there may be minor disturbances. The shape is mostly round, with no apparent elongation.
