The galaxy appears as a relatively smooth, elliptical-like structure with a generally round morphology. A noticeable color gradient is present, transitioning from a more bluish hue in a localized region to a dominant yellowish-red color throughout the main body. This color variation might indicate differing stellar populations or dust distribution within the galaxy.

There is no prominent evidence of distinct spiral arms or a well-defined disk. Faint irregularities might be present, but their prominence is minimal. No clear signs of ongoing major merger activity are observed. The galaxy seems to be largely undisturbed with no significant tidal tails or other obvious distortions. The galaxy possesses an estimated stellar mass that places it within the high end of typical galactic masses. Its rate of star formation appears low to moderate, indicating that star formation is not vigorously active, but is also not completely quenched.
