The galaxy appears to be an elliptical galaxy, characterized by a smooth, spheroidal morphology. The light distribution is concentrated towards the center, exhibiting a high degree of central luminosity. The color profile suggests an older stellar population, with a reddish-yellow core transitioning to a slightly bluer halo. There is no apparent spiral arm structure or significant dust lane obscuration visible. The overall appearance indicates a well-mixed stellar population with minimal ongoing star formation. Any tidal features or signs of recent mergers appear absent, suggesting a relatively relaxed and undisturbed evolutionary history.
