The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. It exhibits a color gradient, appearing generally more yellow in the central regions, indicating a higher concentration of older stellar populations. The outer regions exhibit a bluer tinge, suggesting the presence of some younger stars, though not in prominent spiral arm structures. There is no strong evidence of ongoing major merging events or significant tidal disturbances. The overall morphology appears relatively undisturbed and relaxed. The galaxy displays a moderate redshift, suggesting a considerable distance.