The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a smooth, diffuse morphology with a subtle color gradient, transitioning from a yellowish core to a slightly redder outer region. There is no clearly defined disk or spiral arm structure visible. The central bulge appears dominant, suggesting a relatively old stellar population. There may be evidence of a minor gravitational disturbance, with some slight asymmetry in the light distribution, but no major merger activity is readily apparent. The overall shape is more rounded than elongated.
