The galaxy presents as an elliptical or lenticular type system, with a generally smooth light distribution. There is a highly concentrated, bright central bulge which fades into a more diffuse halo. The galaxy appears elongated in shape, and the primary axis is clearly visible. There's a slight indication of possible minor disturbances, perhaps tidal tails or faint asymmetries, but no strong evidence of a major merger event. Overall, the morphology suggests an evolved system. There are hints of blue light in the outskirts, which may point to regions of ongoing, albeit potentially low-level, star formation, but the dominant color is reddish-yellow, indicating an older stellar population.
