The galaxy appears to be elliptical in shape, exhibiting a high degree of sphericity. It presents a smooth, featureless morphology with no apparent spiral arms or bar structure. The light distribution appears centrally concentrated, gradually fading outwards from the core. The galaxy shows a strong emission in the green portion of the spectrum, with relatively less emission towards the red. There are no obvious signs of ongoing mergers or major disturbances. The galaxy presents a minor distortion in its shape, possibly due to a minor disturbance, but on the whole, it is a very round galaxy.
