The galaxy presents as a largely smooth and rounded structure. The core exhibits a concentrated luminosity, appearing nearly spherical with a noticeable yellow-orange hue. Moving outward from the core, the luminosity gradually decreases, fading into a less defined halo. There is no apparent spiral arm structure or dust lane obscuration visible in the image. Minimal signs of recent or ongoing mergers or tidal disruptions are observed. The overall morphology suggests an elliptical galaxy, possibly of an earlier type given its smooth appearance.
