The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. The core exhibits a bright, diffuse glow, suggesting a high stellar density. Moving outward from the nucleus, the light gradually diminishes into the surrounding halo, with a yellowish hue indicating an older stellar population. There is very little evidence of spiral arms or dust lanes, supporting the classification as an elliptical galaxy. The overall structure appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. The galaxy has a slightly rounded shape. There is no prominent star formation indicated by blue light.
