The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population. Moving outwards from the core, a more diffuse, bluish-white component is observed, possibly indicating regions of younger stars or ongoing star formation, though subtle. The galaxy appears generally well-defined with minimal signs of significant tidal disturbances or interactions with neighboring galaxies, although a minor disturbance cannot be completely ruled out. It is an object of intermediate size and luminosity.
