The observed galaxy presents a generally smooth, elliptical morphology. The core exhibits a high surface brightness, appearing concentrated and nearly circular. Proceeding outward from the core, the light gradually decreases in intensity. There is a small, nearby region with a slight color difference and brightness that could indicate the presence of a minor disturbance, or possibly a background object. Otherwise, the general shape shows a clear lack of spiral arms or a distinct disk-like structure. It appears to be generally isolated.
