The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its overall shape is roughly rounded, exhibiting only a slight elongation. The core region displays a bright, yellowish-white hue, indicating a population of older, lower-mass stars. Moving outward from the core, there's a subtle shift towards greenish-blue tones in the outer regions, hinting at the presence of younger, hotter stars and possibly some ongoing, though weak, star formation. There is no evidence of strong spiral arm structure or significant dust lanes. No signs of major mergers or tidal disturbances are visually apparent. The galaxy appears to be relatively isolated and undisturbed.
