The galaxy presents as a well-defined, elliptical structure. It exhibits a smooth, centralized luminosity profile, with the highest intensity concentrated within the core region. The galaxy displays a moderate ellipticity. There is no apparent evidence of strong tidal interactions or major mergers in progress. Disk-like structure may be present, though it is more likely that the galaxy is elliptical. The light appears to be red-shifted, meaning it may be at a distance from us. Overall, the object has an ovoid shape with no indications of spiral arms or distinct morphological features. The core is very luminous, meaning there is probably a supermassive black hole. The star formation rate is likely low due to the lack of blue light. It is possible this galaxy is in its quiescent phase.
