The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. There is a slight elongation in its shape, appearing more elongated than perfectly circular, but not exhibiting a highly flattened disk structure. The light distribution appears to be generally uniform and lacks prominent spiral arms or strong dust lanes.

The galaxy exhibits a color gradient, with a bluer hue concentrated in the central region transitioning to a redder color in the outer regions. This may imply ongoing or recent star formation in the core, with older stellar populations dominating the outer parts. Alternatively, the central bluer region may be dominated by a strong active galactic nucleus with a relatively weak contribution from the host galaxy. There is no visible evidence of a major ongoing merger, although a subtle asymmetry or faint tidal feature cannot be ruled out. 
