The galaxy presents as a luminous, elliptical-shaped object. Its core exhibits a concentrated, bright yellowish-orange hue, suggesting a population of older stars. The galaxy's luminosity decreases gradually outwards from the central region, transitioning to a less saturated yellowish-orange. There is no apparent spiral structure or dust lanes visible in the image. The galaxy appears generally smooth, with a high degree of symmetry and rotational invariance. There's no obvious indication of tidal tails or morphological disturbances associated with recent major mergers, although there may be some minor asymmetry hinting at a possible minor disturbance or past interaction. The galaxy is intermediate in size compared to other background objects in the image. 
