The galaxy presents a largely smooth, elliptical morphology. It appears quite rounded, displaying minimal visible disk-like structures or pronounced features. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population, likely older stars. The galaxy displays a color gradient, shifting towards redder hues, indicative of a population of evolved stars with a relatively low rate of ongoing star formation. There is no evidence of major mergers or significant tidal disturbances. The galaxy's structure suggests it is a relaxed system that has likely undergone significant evolutionary processes to reach its current state.
