The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a centrally concentrated light profile. Its overall shape is round, lacking any strong features or disturbances indicative of a recent merger or tidal interaction. The color gradient suggests an older stellar population, with the central region appearing more yellow and the outer regions slightly redder. The galaxy's low star formation rate is consistent with its overall morphology and color. It presents no evidence of spiral arms or a prominent disk structure, which aligns with the categorization of an elliptical galaxy. Overall, it is a quiescent system with a high probability of residing on the red sequence.
