This galaxy exhibits an elliptical morphology, appearing largely smooth and concentrated. The light distribution suggests a spheroidal structure, with a gradual decrease in intensity from the center outwards. There is some indication of minor asymmetry or perturbation in the outer regions, hinting at possible past or ongoing interactions. The galaxy presents a redder hue, indicative of an older stellar population and a relatively low rate of ongoing star formation. Overall, the object is consistent with a mature galaxy that has undergone significant evolution.
