The galaxy presents a generally smooth, elliptical appearance, suggesting an older stellar population. The light is concentrated towards the center, which has a yellow-orange hue. This contrasts slightly with the less dense outer regions, which exhibit a redder color. There is no clear evidence of a spiral structure or significant dust lanes. Some minor asymmetry is present, hinting at the possibility of past interactions, but the overall structure is undisturbed. There is no nucleus visible.
