The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a high degree of luminosity, appearing almost uniformly bright and yellowish-white. The light intensity decreases gradually outwards from the core, forming a diffused halo. There is a slight elongation visible in the galaxy's shape, deviating from a perfect circularity and more towards an in between rounded shape, suggesting a weak disk-like structure. There is no apparent spiral arm structure or significant dust lane presence visible in the image. The morphology is suggestive of an early-type galaxy with minimal recent or ongoing major merging activity.