The galaxy presents as a fairly smooth and centrally concentrated object. Its overall morphology appears elliptical or spheroidal, with a high degree of roundness. The light distribution is consistent with a system dominated by an older stellar population, indicated by its reddish-yellow hue, with the bluer light suppressed. There's no clear evidence of spiral arms, bars, or significant dust lanes. There appears to be no major ongoing merger activity or significant tidal disturbances affecting the galaxy's overall structure. The galaxy appears to be an isolated system.
