The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population. Moving outward from the center, a faint blue-green halo surrounds the core, possibly indicating areas of more recent, though subdued, star formation. The overall shape appears moderately elongated. There is some evidence of asymmetry and possible tidal disturbances. This indicates a potential recent or ongoing interaction with another galaxy, possibly in the form of a minor disturbance or merger event. The galaxy does not display a clear spiral structure.
