The galaxy presents a largely smooth, elliptical morphology. Its color profile exhibits a dominant yellowish-orange hue, suggesting a stellar population primarily composed of older, evolved stars. The central region of the galaxy appears brighter and more concentrated than the outer regions. There is a subtle flattening to the disk, and possibly a very weak bar. There is a possibility of some minor gravitational disturbance, but for the most part it does not appear to be merging or interacting with any other galaxies. The absence of significant blue coloration indicates a low rate of recent star formation.
