The galaxy presents as a moderately bright, centrally concentrated object. It appears largely featureless, with a smooth light distribution, suggesting a dominant spheroidal component. The color is generally yellowish, indicative of an older stellar population. The galaxy exhibits a generally round morphology. There is no clear evidence of a spiral arm structure. Its estimated physical size is consistent with a large galaxy. The galaxy displays no signs of major disturbances or ongoing mergers, though there are some hints of minor tidal interactions or disturbances, but most likely this galaxy has not experienced a major merger event recently.
