The galaxy presents a generally smooth, elliptical morphology. There is a noticeable central bulge which appears to be the brightest and most concentrated region. The color profile indicates an older stellar population, as evidenced by the reddish-orange hue dominating the core and inner regions. The galaxy appears relatively undisturbed, with no prominent tidal features or asymmetries visible, although there seems to be a slight elongation along its major axis, presenting an in-between roundness. The galaxy is likely not actively merging with another galaxy. Overall, this galaxy exhibits characteristics consistent with a relatively massive, quiescent system with a low star formation rate.
