The galaxy presents an elliptical morphology, appearing generally smooth with no obvious spiral arm structure. The central region exhibits high surface brightness, indicative of a dense stellar population or active galactic nucleus. A gradual decrease in luminosity is observed from the core outwards, forming a diffuse halo surrounding the nucleus. The color profile suggests an older stellar population dominating the overall light emission, leaning toward redder wavelengths. There is no distinct dust lane or prominent star-forming region visible within the galaxy's structure. It appears largely undisturbed, showing no strong tidal features or signs of recent major merger events.
