The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The color profile suggests an older stellar population, appearing redder in color. There is no visible evidence of spiral arms or active star formation regions. The galaxy appears to be isolated, showing no significant signs of tidal disturbances or interactions with other galaxies. The overall form indicates that it is not an actively merging galaxy. The shape appears mostly round.
