The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a yellowish hue, suggesting an older stellar population. The outer regions display a gradient towards bluer tones. The galaxy appears generally undisturbed, without prominent tidal features or indications of a recent major merger, although there are some signs of minor disturbances in the outer disk. The overall form suggests a mature galaxy, potentially with ongoing, but not intense, star formation.
