The galaxy appears as a centrally concentrated, generally smooth object. It exhibits a predominantly elliptical morphology with a high degree of roundness. The galaxy displays a radial color gradient, appearing more yellow-orange at the core, suggestive of an older stellar population in the central regions. There is no discernible spiral structure or prominent dust lanes. There are also no clear signs of any major ongoing merger activity or tidal disturbances; any disturbances that may be present appear minor.
