The galaxy presents as a largely smooth, elliptical-like object, with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the central region. The overall shape is close to round. Subtle color gradients are visible, with a slight reddening observed in the outer regions, possibly indicative of a more metal-rich or dustier environment away from the nucleus. There is no obvious spiral arm structure or prominent dust lanes. The galaxy appears relatively undisturbed, showing no significant signs of tidal interactions or ongoing major mergers, with a small, minor disruption in the form of a very small tail to the left of the core. The overall impression is that of a mature galaxy, likely undergoing minimal star formation.
