The galaxy presents a largely smooth morphology. It appears elliptical in shape, exhibiting a high degree of central concentration with a bright core. The color profile suggests a population of older stars, as indicated by its yellowish-red hue. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly bluer, possibly hinting at a minor component of younger stars or low-level star formation activity. No prominent spiral arms or dust lanes are discernible within the visible structure of the galaxy. The overall impression is that of a relatively quiescent, evolved system. Subtle disturbances in the galaxy's structure cannot be fully ruled out, but they are not immediately apparent in the provided image.
