The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light distribution. It exhibits a near-spherical morphology with no discernible spiral arm structures or prominent dust lanes. The color profile indicates a yellow-orange hue, suggesting an older stellar population and a relative lack of ongoing star formation. The galaxy displays a gradual radial decrease in surface brightness, with a diffuse outer halo. There are no apparent signs of tidal interactions or major disturbances in its overall structure. The galaxy's profile indicates it is quite massive.