The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing bright and slightly yellowish-white. Moving outwards from the core, there's a gradual decrease in luminosity, transitioning into a bluer hue. The overall structure suggests a relatively evolved system, with a significant fraction of its stellar population being older. There are hints of possible minor disturbances in the outer regions, potentially indicating past or ongoing interactions, though no clear signs of major mergers or tidal tails are apparent. The galaxy's round appearance indicates that if it is a spiral galaxy it is seen close to face on.
