The galaxy appears to be a relatively compact, elliptical system. Its light is dominated by a smooth, spheroidal component. The color profile suggests an older stellar population with minimal ongoing star formation, indicated by the yellow-red hue. There is a bright central concentration of light, with no obvious dust lanes or spiral arm structures visible. The overall morphology suggests a relaxed system with a high degree of symmetry and minimal signs of recent interactions or mergers. There is a faint, diffuse halo surrounding the main body of the galaxy.
