The galaxy presents as a centrally concentrated elliptical. It has a smooth, diffuse appearance lacking prominent spiral arms or a distinct disk structure. The core region is bright and elliptical, suggesting an older stellar population. There is a slight color gradient, with the core appearing more yellow, which could be the result of a higher concentration of older, redder stars, and the outer regions appearing somewhat bluer, potentially indicating more recent star formation at its edges, or younger stars in the outer regions. The galaxy's shape appears to be largely spheroidal with a hint of elongation along one axis. There appears to be another object nearby that could be interacting with the galaxy. The galaxy is generally isolated.
