The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated core is observed. The overall color profile suggests a relatively evolved stellar population, skewed towards longer wavelengths, as indicated by the apparent yellowish hue. Faint extensions are visible on either side of the core, which may suggest a weak disk or tidal features. The structure appears relatively undisturbed, with no obvious signs of major merging events or strong tidal distortions. The galaxy does not seem to have well-defined spiral arms.
