The galaxy appears to be a relatively smooth, elliptical or lenticular type. It presents a centrally concentrated bulge, exhibiting a bright, redder hue. A less prominent, slightly bluer halo surrounds the central region. The overall morphology is generally round. There is no visual evidence of significant spiral arm structure, nor is there a clear indication of ongoing major merger activity or tidal disturbances. The galaxy's disk, if present, is seen at a shallow angle. Based on the light profile, it could be inferred that star formation is present at a low level, or recently diminished, as evidenced by the bluer color of the outer region compared to the core. The galaxy presents a moderate size, and is observed at redshift z=0.19.
