The galaxy appears to be a relatively smooth, elliptical system with a slightly elongated morphology. The core region presents a concentrated, luminous intensity, which decreases gradually towards the outer edges. The color profile indicates a dominance of older stellar populations, exhibiting a yellow-orange hue. There is no discernible dust lane, spiral arm structure, or evidence of intense star formation activity. Minor asymmetrical features are seen in the outskirts, hinting at possible interactions or past merger events, although the primary structure appears largely undisturbed. Overall, the system presents itself as a galaxy in a relatively advanced stage of its evolutionary trajectory.
