The galaxy presents a largely smooth and concentrated morphology. The light profile indicates a centrally dominant bulge component, with a gradual decrease in surface brightness moving outwards. The overall color is slightly redder in the core, transitioning to somewhat bluer hues in the outer regions, suggesting a radial gradient in stellar populations. The shape appears to be generally elliptical, displaying minimal signs of strong tidal distortions or interactions that would indicate a recent or ongoing merger event. There might be some minor disturbances in the shape, but they could also be image artifacts. The central region is intensely bright, implying a high concentration of stars, possibly including an actively star-forming population or an active galactic nucleus. Star formation is estimated to occur in the galaxy. The overall characteristics suggest that this galaxy is relatively massive.
