The galaxy appears as a relatively compact, elliptical-like structure. Its color profile indicates a concentrated central region of older stars, exhibiting a yellowish hue. The outer regions show a slight decrease in yellow with a subtle hint of blue, which implies the presence of some younger stellar populations, possibly due to ongoing or recent star formation activity within its disk. Overall, the galaxy presents a smooth and largely undisturbed morphology, with no obvious signs of tidal features or major merger events in its recent past. There might be a very small, almost indiscernible disk structure surrounding the core.
