The galaxy presents as a relatively compact object. Its morphology appears predominantly smooth, with no discernible spiral arm structures or a prominent central bar. The light distribution is centrally concentrated, fading gradually towards the edges. Color gradients are subtle, with a slightly bluer hue in the outer regions, potentially indicating younger stellar populations, and a redder core, suggestive of older stars. The galaxy's shape is somewhere in between round and elongated. There appears to be no major merging events or severe tidal disruptions, although the smoothness is subtly disturbed, suggesting minor perturbations.
