The galaxy presents as a relatively compact and luminous object, likely with a substantial stellar mass. It appears primarily smooth in structure, indicative of an elliptical galaxy, though there seems to be a hint of a disk structure. The main body is characterized by a somewhat rounded shape with very little asymmetry, suggesting a dynamically relaxed state. There is some evidence of a possible minor interaction or merger event, as indicated by some small distortions in the outer regions. The color suggests that it is composed mostly of older stars, likely with a suppressed star formation rate. 
