The galaxy presents as a single, relatively smooth object. Its morphology appears largely elliptical, with a high degree of roundness observed. The core region exhibits a concentrated, yellowish-white hue suggesting an older stellar population. The galaxy exhibits a significant red shift and a low star formation rate. It's estimated to be massive. Faint, diffuse extensions of the galaxy are potentially visible beyond the central core, though they are poorly resolved. There is no apparent spiral arm structure nor any signs of any major mergers or tidal disturbances visible in this imaging.
