The galaxy presents as a single, relatively symmetrical and compact object. The light distribution appears largely smooth and centrally concentrated. Its morphology is generally elliptical or spheroidal, lacking any distinct spiral arm features or prominent bars. The galaxy exhibits a color gradient, with a more yellowish-red hue in the central region, transitioning to a slightly bluer tint towards the outer edges. This may be due to differential stellar populations. There are no visible signs of ongoing major mergers, tidal tails, or significant disk-like structures, although some minor disturbances cannot be completely ruled out based on this image alone. Its overall appearance is consistent with that of a mature elliptical galaxy or a lenticular galaxy viewed face-on. 
