The galaxy presents a generally smooth and rounded morphology. There is little evidence of significant spiral arm structure or a distinct disk. The light distribution appears relatively uniform across the galaxy's body, with a concentration towards the center. Given the overall smooth appearance, the galaxy is potentially an elliptical galaxy with a substantial stellar mass and old stellar populations. The color profile suggests that star formation activity is largely quiescent. The apparent lack of any major disturbances implies that the galaxy has not recently undergone a significant merger event, and is more likely to have undergone minor disturbances.
