The galaxy exhibits a generally elliptical morphology, appearing largely smooth and lacking in prominent spiral arm structures or significant dust lanes. The galaxy's color profile suggests a relatively evolved stellar population, with a dominant yellowish-red hue in the central region that fades to a slightly bluer cast towards the outer edges. This could indicate a concentration of older, redder stars in the galactic bulge, with some ongoing, or recent, star formation occurring in the periphery. There is no indication of a significant ongoing merger event. The overall structure presents as highly concentrated.
