The galaxy presents a largely smooth morphology with a concentrated central region. The light distribution appears relatively elliptical, displaying a slightly elongated shape. A color gradient is observable; the core exhibits a warmer hue, trending towards redder wavelengths, which may indicate an older stellar population or dust obscuration. Moving outwards from the core, the color shifts towards bluer tones, potentially indicative of younger, hotter stars in the outer regions, or a different, less dust-obscured stellar population. There is some faint indication of possible disturbances in the galactic disk or halo, but overall the galaxy seems relatively undisturbed with no clear signs of a major ongoing merger. The galaxy displays a soft, diffuse halo.
