The galaxy exhibits a generally elliptical morphology, appearing slightly elongated. The central region displays a high surface brightness, suggesting a concentrated stellar population or active galactic nucleus. Moving outward from the core, the surface brightness diminishes, transitioning into a more diffuse halo. There appears to be some slight asymmetry in the outer regions, possibly indicating tidal disturbances or interactions with smaller satellite galaxies. The overall color profile suggests a relatively mature stellar population. I do not see any distinct spiral arms or obvious signs of recent major merger events.
