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   <subfield code="a">We present the results of our infrared J H K L photometry of the Seyfert galaxy NGC 4151 during its active period in 1995-2011. The variable IR source was still in its active state in 2011, though its observed luminosity had almost halved compared to the maximum of 1995-1996. If the &quot;cool” component of the galaxy's variable source is a dust shell heated with the central &quot;hot” source, its optical depth at 1.25 µm varied from 0.3 to almost 1.0, its temperature from 700 to 950 K, its size from 20 to 40 pc, and its mass from 2 to 40M ⊙ during our observations. A component with a period of 317 ± 5 days can be revealed in the flux variations observed in 1994-2011.</subfield>
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