The galaxy presents a generally smooth, elliptical morphology. It appears relatively round, showing minimal elongation. A slight central concentration of light is visible, though not overly pronounced. The galaxy exhibits a subtle color gradient, with a bluer hue towards the core transitioning to a redder, more diffuse halo region. There is potential evidence of a minor interaction or disturbance in the galaxy's structure, possibly a faint tidal feature or asymmetry. The overall appearance suggests a system undergoing relatively low levels of star formation, consistent with a more evolved, passive galaxy.