The galaxy presents as a singular, relatively smooth, elliptical structure. The color profile suggests an older stellar population. The lack of significant color variation across the galactic body indicates a dearth of recent star formation activity. It exhibits a somewhat round profile. There is no strong evidence of a major ongoing merger event, but there are hints of minor disturbances in the outer regions of the galaxy, possibly indicating past interactions or accretion events. The apparent size suggests a moderately large galaxy.
