The galaxy presents as a single, largely homogenous structure. Its overall form appears relatively smooth, lacking any distinct spiral arms or bar features. The light distribution is centrally concentrated, with a gradual falloff in intensity towards the outer regions. The galaxy exhibits a subtle color gradient; the core region displays a yellowish hue, which transitions towards a bluer tone in the outer regions. The overall ellipticity appears minimal, suggesting a nearly circular or slightly flattened spheroidal shape. There is no clear evidence of ongoing major mergers or significant tidal disturbances. The galaxy seems to be a relatively undisturbed system, exhibiting a high degree of symmetry and regularity in its morphology.