The galaxy appears to be a relatively smooth, elliptical system. The central region exhibits a high concentration of light, appearing bright and somewhat reddish-orange in color. The galaxy appears to be slightly elongated in shape, with a clear major axis. There's a smooth decrease in light intensity moving outwards from the center towards the outer regions. A faint greenish-yellow halo surrounds the central region, extending outwards with decreasing intensity. There is little evidence of spiral arm structure or significant dust lanes, suggesting an older stellar population and a relatively quiescent star formation rate. The overall structure suggests a galaxy that has undergone significant merging or internal dynamical relaxation.
