The galaxy presents as a luminous elliptical structure, elongated along a major axis oriented approximately horizontally in the image frame. The central region exhibits a high surface brightness, appearing nearly spherical with a slight concentration. Moving outward from the core, the light distribution becomes more diffuse, fading into the background sky. There is evidence of tidal features and possible ongoing merger activity, with a slightly disturbed morphology and irregular features. It appears that there is some evidence of past mergers or gravitational interactions, resulting in a somewhat irregular shape.
