The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated light profile, with a core region that is slightly redder in color, suggesting an older stellar population. Moving outward from the core, the light becomes slightly bluer, possibly indicating the presence of younger stars, although this could also be due to differences in dust extinction. No distinct features such as spiral arms or a bar are discernible; the galaxy possesses a generally featureless morphology. There is no significant evidence of tidal disturbances or interactions with other galaxies. The object seems to be an isolated system in a relatively relaxed state, as no obvious signs of recent mergers or accretion events are visible.
