The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright yellow hue indicative of an older stellar population. A gradual color gradient transitions from the core toward the outer regions, where the color shifts towards greenish blue, suggesting the presence of some younger, hotter stars. However, the overall light distribution indicates that star formation is suppressed. The galaxy displays a moderate degree of roundness, deviating slightly from a perfectly circular shape, with a hint of asymmetry in its overall structure. There appear to be some tidal features or minor distortions in the galactic disc structure.
