The galaxy presents as a largely smooth, elliptical structure. The color profile suggests a dominant population of older stars, potentially indicating a lower rate of ongoing star formation. The galaxy is essentially spheroidal, with a slight deviation from perfect circularity. There is no immediately visible evidence of spiral arm structures or a distinct galactic disk. Furthermore, the structure displays no obvious signs of major mergers or significant tidal disturbances, although the possibility of a minor past interaction cannot be entirely ruled out based on this image alone. The observed characteristics, including its color and overall shape, imply that the galaxy is a reasonably massive system.
