The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a centrally concentrated light profile. The core region is bright and gradually fades towards the outer edges. There's a hint of a slight blueish hue in the outer regions, which may indicate some low level of recent star formation. The overall structure suggests that it is well relaxed and potentially contains older stellar populations. No distinct spiral arms or bar structures are visible, supporting its classification as an elliptical galaxy. The morphology shows a high degree of roundness in the central regions. There is no evidence of any major merging events, but some minor asymmetries could suggest past or ongoing interactions.
