The galaxy presents as a relatively smooth, elliptical-like structure. The color profile suggests a higher concentration of older stellar populations, as indicated by the reddish-yellow hue. There is no apparent disk structure or spiral arm morphology visible in this observation. There are no major disturbances or signs of ongoing mergers observed. The galaxy appears relatively isolated and undisturbed, although it displays a small amount of asymmetry and irregularities. Its compactness and color suggest a lower star formation rate. Overall, the galaxy appears to be a quiescent, relatively evolved system.
