The galaxy appears to be a relatively smooth, elliptical galaxy at an approximate distance as calculated via redshift to be fairly local. The light profile is centrally concentrated, with the bluest light emanating from the core, suggesting some recent, though likely low level, star formation activity occurring within that region. The light exhibits a slight elongation. The surrounding halo of older stars transitions smoothly outward, becoming redder. There is no readily apparent evidence of strong tidal interactions or major disturbances, though there is a faint hint of asymmetry or minor disturbance in the outer isophotes, possibly due to a past minor merger. The galaxy seems to be generally isolated within its immediate surroundings.
