The galaxy exhibits a generally smooth, rounded morphology, suggesting an elliptical or lenticular classification. The light distribution appears relatively uniform across the galaxy's body, indicating a lack of prominent spiral arms or distinct features. A slight color gradient is observable, trending towards redder hues centrally and bluer tones in the outer regions. This could imply a higher concentration of older stellar populations in the core, with younger, bluer stars populating the outskirts. There is some minor asymmetry present within the galaxy's halo, which may indicate a past interaction or tidal disturbance. Its overall structure is not significantly distorted.