The galaxy presents as a relatively smooth, centrally concentrated object. Its color profile appears to be redder, suggesting a population of older stars with lower ongoing star formation. There is a high degree of overall symmetry to the galaxy, with an elliptical morphology, with the galaxy appearing rather round with no obvious extensions or tidal features. There is no substantial evidence of a distinct disk structure. The overall appearance suggests an evolved system possibly a massive elliptical galaxy. There are no signs of ongoing major merging activity or significant disturbances in the galaxy's structure.