The galaxy appears to be a relatively smooth, elliptical or lenticular type system. It presents a centrally concentrated bulge that fades outward into a more diffuse halo. There is no immediately obvious spiral structure or distinct dust lanes visible in this image, supporting the smooth classification. The overall color seems relatively uniform across the galaxy, suggesting a stellar population dominated by older stars. There are no indications of active star formation regions, such as HII regions or blue star clusters, which would appear as bright, blue knots. While there is an appearance of slight distortion from the round nature of the galaxy, it generally shows no major signs of recent interactions or mergers, although a minor disturbance can not be ruled out.
