The galaxy presents a largely smooth and centrally concentrated morphology. It appears elliptical in shape, displaying a high degree of circular symmetry. The central region is characterized by a bright, yellowish hue suggesting an older stellar population. Moving outward from the core, a gradual color shift towards bluer tones is observable, possibly indicative of younger stars and ongoing star formation within the outer regions. There is a subtle hint of a disk component although it is not very clear. The overall structure suggests a quiescent galaxy, though some minor disturbances cannot be ruled out.
