The galaxy presents as a single, relatively smooth object with a noticeable central concentration of light. The overall shape is elliptical, appearing somewhat elongated but predominantly round, displaying a smooth gradient in luminosity from the center outwards. The core exhibits a reddish hue, possibly indicative of an older stellar population. Surrounding the core, there is a greenish-yellowish halo that extends outwards, suggesting the presence of a younger, bluer stellar population or ionized gas. There is no obvious spiral structure, bar, or other distinct features; nor is there any clear evidence of a major ongoing merger. The galaxy appears relatively undisturbed, though a very slight asymmetry cannot be ruled out given the image quality.
