The galaxy presents a generally smooth and centrally concentrated morphology. The central region exhibits a high surface brightness, appearing nearly spherical and gradually fading into the outer regions. There's a subtle elongation to the galaxy's shape; it's not perfectly circular. The overall color profile suggests a population of older stars, with a yellowish-red hue dominating, which is characteristic of galaxies with suppressed star formation. There are subtle signs of disturbances, though generally they are minor. There is no obvious grand design spiral structure.
