The galaxy appears to be a relatively smooth, elliptical galaxy with a slightly elongated shape. It presents a bright, centrally concentrated core that fades into a more diffuse halo. The color profile indicates a generally older stellar population, as suggested by the reddish-yellow hue, but there is also evidence of blue light emission within the central region indicating at least some ongoing star formation. No distinct spiral arms or prominent dust lanes are visible. There is a hint of tidal disturbance on the edges, but the galaxy appears mostly undisturbed.
