The galaxy presents as a largely smooth, elliptical-like structure. It appears relatively featureless with a high degree of central concentration. The galaxy exhibits a somewhat round morphology. The galaxy's light profile appears to decrease smoothly and monotonically from the core outward. There is no evidence of significant tidal disturbances, major mergers, or prominent disk features. The galaxy appears to be a relatively quiescent system in terms of star formation. Overall, the galaxy appears to be a relatively isolated, undisturbed system.
