The galaxy presents a relatively smooth, centrally concentrated light distribution. Its morphology appears largely elliptical or spheroidal, with minimal evidence of spiral arms or a distinct disk component. The galaxy exhibits a generally rounded shape, though some slight deviation from perfect circularity may be present. The galaxy's color profile suggests a evolved stellar population, as indicated by a relative brightness in the redder bands. There are no clear signs of major mergers or tidal disturbances. The galaxy seems to be a non-disturbed system.
