This source is a **low-luminosity radio galaxy of FR I type**, hosted by an **elliptical galaxy** (likely massive, gas-poor), with no evidence of strong star formation or quasar-like activity.

Key evidence:  
- Radio morphology is classified as *FR I (Complex)* in both files, confirmed by high-resolution VLA imaging showing edge-darkened, collimated jets that fade toward the lobes—characteristic of sub-relativistic, turbulent jets decelerating in a dense ambient medium.  
- The *Peak Inside* and *Zero Peak Offset* (Peak_Offset_Arcsec = 0) indicate the radio core coincides precisely with the optical/near-IR host position—ruling out significant jet misalignment or double-lobe displacement typical of FR II or restarted sources.  
- DC_Maj = 12.5″ (deconvolved major axis) at BMAJ = 2.9″ beam implies a physical size ~30–50 kpc at typical FR I redshifts (z ≈ 0.05–0.1), consistent with nearby ellipticals.  
- Low Flux_Ratio (0.0833 in second file) reflects minimal lobe-to-core flux—another FR I hallmark, distinguishing it from FR II (high lobe/core ratio) or starbursts (diffuse, unstructured emission).  
- SNR = 7.1 is sufficient for robust morphological classification but too low for a bright quasar or blazar; absence of UV/X-ray/IR multiwavelength data here does not contradict this, as FR I nuclei are typically radiatively inefficient (ADIOS or ADAF accretion), lacking strong thermal disk emission or dust-obscured starburst signatures.

No indication of spiral structure, starburst IR colors, or broad emission lines—thus, **elliptical-hosted FR I radio galaxy** is the most physically consistent classification.