The galaxy presents a relatively smooth, concentrated light profile. It appears elliptical in shape, tending towards an intermediately rounded form rather than a perfectly circular or elongated shape. The galaxy's core exhibits a brighter intensity compared to its outer regions, indicative of a centrally concentrated structure. There's a subtle suggestion of minor disturbances or irregularities in its structure, though a clear merging event is not definitively indicated. Overall, the galaxy's morphology suggests it is a relatively undisturbed system without significant signs of ongoing major mergers or tidal interactions.
