The galaxy presents as a smooth, elongated structure. Its morphology suggests it is likely an elliptical galaxy. There is a distinct central bulge that is brighter and more concentrated than the surrounding regions. The light appears to smoothly fade outwards from the core, exhibiting a diffuse halo with no apparent spiral arm structures or significant dust lanes. The color is generally uniform, with a slightly redder hue overall, consistent with an older stellar population and reduced star formation. There is no evidence of active galactic nuclei activity in this image, given the lack of intensely bright and concentrated emission. The overall impression is of a relatively quiescent, evolved system.
