The galaxy presents a roughly elliptical morphology. The central region exhibits a high surface brightness, appearing nearly circular and predominantly yellow, likely indicating an older stellar population. The outer regions of the galaxy show a more diffuse structure, with a blue tint. The smooth appearance, as well as the colors, suggest that there is some star formation going on, but at a very low rate compared to its mass. Possible minor disturbances visible in the outer structure could be evidence of a recent or ongoing merger. However, there are no large tidal tails or strong asymmetries visible, suggesting any interaction is either ancient or relatively minor in scale.
