The galaxy appears as a singular, luminous entity with a largely homogenous structure. Its form is overwhelmingly elliptical, showing a high degree of central concentration of light. The galaxy is generally a warm yellow color, with hints of green, that likely suggests an older stellar population dominating the light emission, with minimal ongoing star formation. There is a slight red area slightly offset from the center of the galaxy, that suggests a small amount of dust extinction, or potentially a region of older, redder stars. There is no evidence of spiral arms or a distinct galactic disk, nor any signs of significant tidal disturbances or ongoing merger events. The galaxy appears generally relaxed and undisturbed, which is consistent with its morphology.
