The galaxy presents an elliptical morphology, appearing relatively smooth in overall structure with a moderate degree of central concentration. The light distribution exhibits a noticeable bulge component, with a gradual decrease in surface brightness moving outward from the core. There is a slight hint of a possible disk-like structure. The galaxy appears to be undergoing a minor interaction with a companion galaxy, showing some evidence of tidal disturbance or asymmetry in its outer regions. This interaction is potentially triggering elevated levels of star formation, particularly in the core of the galaxy. The overall color is yellowish-white, indicative of a stellar population that is primarily older, but with possible younger, bluer stars present in the core. The galaxy is a moderate size and mass.
