The galaxy presents as a centrally concentrated, relatively smooth structure with a slightly elongated morphology. The central region exhibits a bright, compact core with a high degree of symmetry. There appears to be a subtle color gradient from the center outwards, with the core exhibiting a bluer hue that gradually shifts toward a redder tone in the outer regions. While the bulk of the light is centrally concentrated, there is some evidence of a more diffuse, extended halo surrounding the core. Visual inspection does not clearly reveal any strong spiral arm features, bars, or other pronounced morphological substructures. The overall impression is that of a relatively evolved system, potentially an elliptical or lenticular galaxy. Subtle irregularities in the outer isophotes suggest possible minor interactions or disturbances.
