The galaxy presents an elliptical morphology, with a smooth, centralized concentration of light that decreases gradually toward the outer regions. The major axis is oriented at a position angle of approximately 135 degrees. A color gradient is observed, with the core exhibiting a more yellow to orange hue that suggests an older stellar population, while the outer regions appear slightly bluer. The galaxy shows no obvious spiral arm structures or dust lanes. It displays a relatively high degree of symmetry. The overall appearance is indicative of a galaxy undergoing a low rate of star formation.
