The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears reddish-pink in color, suggesting a population of older, redder stars. Moving outward from the core, a diffuse, greenish halo surrounds the central region. This greenish hue hints at the presence of some ongoing star formation, although it appears subdued. The galaxy lacks any obvious spiral arm structure or significant dust lanes. The overall shape deviates slightly from perfectly circular, showing a hint of elongation. There are no obvious signs of tidal disturbances or interactions with other galaxies, but minor disturbances cannot be ruled out.
