The galaxy presents a largely smooth, elliptical morphology. A central bulge region is prominent, displaying a concentrated luminosity gradient. The galaxy appears to be yellowish-white in color, suggesting a population of older stars. There is minimal visible dust or gas. The overall structure indicates a system that has likely undergone significant merging or relaxation processes in its history. The image indicates a galaxy that is relatively isolated. Based on these characteristics, the object is likely a relatively massive elliptical galaxy with limited current star formation.
