The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a high degree of roundness. The core exhibits a bright, yellowish hue, indicating a population of older stars and potentially a supermassive black hole at the center. A faint, diffuse halo surrounds the core, fading into the background. There is some evidence of minor disturbance in the morphology, but no clear sign of an ongoing major merger. Faint blue hues are present toward the edges of the galaxy, suggesting the existence of younger stars in the outer regions. Overall, the galaxy appears to be an early-type galaxy that is no longer actively forming many stars.
