The galaxy appears to be elliptical, with a smooth, concentrated distribution of light. Its core exhibits a bright, yellowish-orange hue, indicating a population of older stars. There is a gradual decrease in luminosity moving outward from the center, with no distinct spiral arm features or significant dust lanes visible. The outer regions of the galaxy present a more diffuse and less defined edge. The overall shape is generally round. There is no obvious sign of any major ongoing merger. The image suggests that the galaxy is relatively quiescent with a low star formation rate.
