The galaxy presents as a single, relatively smooth object with a concentrated central region. There is a clear radial color gradient, with the core appearing more yellow-orange and the outer regions trending towards a bluer hue. The ellipticity appears moderate, with the galaxy exhibiting a somewhat rounded shape rather than a highly elongated one. There is no obvious visual evidence of spiral arms or a prominent disk structure. Minimal signs of tidal disturbances or ongoing merger activity are present. The overall appearance is consistent with a fairly evolved system exhibiting a significant population of older stars in its core, and relatively little ongoing star formation.
