The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated morphology with a diffuse halo. The color profile suggests a dominant population of older stars, contributing to its reddish hue. There is little evidence of spiral arms or significant dust lanes. The galaxy appears largely undisturbed, showing no major signs of an ongoing merger or tidal interaction, although very minor disturbances cannot be ruled out. The overall shape is close to circular, showing only a slight ellipticity.
