The galaxy presents as a relatively compact, elliptical structure, with a smooth, diffuse light distribution. The primary body exhibits a largely homogenous color gradient shifting from a central, yellow hue towards a slightly redder periphery. While generally round, there is a faint elongation along one axis. A smaller, secondary body of lower surface brightness and redder color lies closely adjacent to the primary body. The morphology appears to be characteristic of a galaxy undergoing a minor interaction or possible merger event. Some minor distortions are present and visible, indicative of tidal forces or gravitational disturbances. The central region appears concentrated, while the outer edges fade gradually into the background sky. 
