The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. It is largely spheroidal, with isophotes that are close to circular, showing a slight deviation. The core region emits strongly in the redder wavelengths, suggesting an older stellar population dominated by red giants. Moving outward from the core, the galaxy exhibits a gradual decrease in surface brightness. The faint, outer regions show hints of younger, bluer stars. There are no clear signs of spiral arms or a prominent disk structure, suggesting this is likely an early-type galaxy. The object appears relatively undisturbed, with no obvious tidal features or signs of a recent major merger event. There is a subtle colour gradient from the core to the outer regions, indicating that there is some amount of on-going star formation.
