The galaxy presents an overall elliptical morphology, appearing mostly smooth and concentrated towards the center. There is a slight hint of disk-like structure with some irregularity. The color profile suggests a dominant population of older stars, indicated by a relatively red color, with a hint of younger, bluer stars within the disk. Some disturbance is visible, it does not seem to be a major merger. The galaxy appears to be in a relatively quiescent state of star formation.