This galaxy appears to be an elliptical galaxy, exhibiting a smooth, rounded morphology. There is no visible disk component or spiral arm structure. The galaxy's light profile suggests a concentrated core with a gradual decrease in luminosity towards its outer regions. The color indices suggest that the galaxy is dominated by an older stellar population, with a relatively low rate of star formation. There is no evidence of any major merger events or significant tidal disturbances, however there might be some minor disturbance events. The overall appearance points to a relatively quiescent galaxy that has largely completed its star formation.
