The galaxy appears as an elliptical structure exhibiting a smooth morphology. Its color profile suggests a mix of stellar populations, with a notable concentration of older, redder stars in the central bulge region. The outer regions are less defined, fading into the background sky. The shape is not perfectly spherical, exhibiting a slight elongation. Possible minor disturbances in its structure are present, indicating potential interactions with other celestial objects, though no major merger events are immediately apparent.
