The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated, bright yellowish-white luminosity, suggesting a significant population of older stars. Moving outward from the core, the galaxy appears to fade into a reddish hue, and it is generally devoid of any strong spiral arm structures or prominent dust lanes. The apparent roundness of the galaxy indicates a low inclination angle relative to our line of sight. There are no obvious signs of major mergers or tidal disturbances in this image, the galaxy appears to be in a relatively undisturbed state. It displays a high degree of central concentration, and the colour gradient towards the outer regions is suggestive of an aging stellar population, consistent with a relatively low star formation rate.
