The galaxy presents a largely elliptical morphology with a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, possibly indicative of an older stellar population dominating the central region. Moving outward from the core, a subtle transition towards a greenish-blue coloration is observable, suggesting a younger population of stars and ongoing, albeit subdued, star formation in the galaxy's outer regions. The overall structure appears relatively undisturbed, showing no obvious signs of recent major merger events or tidal interactions. There might be faint hints of a very subtle, diffuse disk component, but it is not prominent and the dominant morphology is smooth and spheroidal. The galaxy appears fairly compact and unresolved.
