The galaxy appears to be elliptical in shape, displaying a smooth, featureless morphology. The core region exhibits a strong concentration of light, suggesting a dense stellar population. A gradual decrease in surface brightness is observed moving outwards from the center. There is a slight yellow tint to the core region. There is no evidence of prominent spiral arms or a central bar structure. Minor asymmetry can be observed on the outskirts, suggesting the possibility of a past interaction, but no significant tidal tails or merging features are seen. The overall color profile suggests an older stellar population, with relatively little ongoing star formation.
