The galaxy presents a largely smooth and rounded morphology, suggesting an elliptical type, viewed face-on. Its color exhibits a central concentration of yellowish-orange hues, indicative of an older stellar population. The outer regions transition to slightly bluer tones, possibly suggesting younger star formation, though at a very subdued rate. There is no discernible disk structure or spiral arm pattern evident in the image. Minor asymmetric distortions are present, perhaps suggesting a past or ongoing minor interaction or merger event, though the galaxy maintains a generally relaxed appearance. Overall, the galaxy appears to be a massive system with an estimated size around 10 kpc and a very low rate of star formation.
