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We report on the discovery of a boxy/peanut shaped bulge in the highlyinclined barred Seyfert 2 galaxy NGC~7582. The peanut shape is clearly evidentin near infrared $JHK$ images but obscured by extinction from dust in visible$BVR$ images. This suggests that near infrared imaging surveys will discover alarger number of boxy/peanut morphologies than visible surveys, particularly ingalaxies with heavy extinction such as NGC~7582. The bulge in NGC~7582 exhibitsstrong boxiness compared to other boxy/peanut shaped bulges. If the starburstwas mediated by the bar, then it is likely that the bar formed in less than afew bar rotation periods or a few $\times 10^8$ years ago. If the bar alsocaused the peanut, then the peanut would have formed quickly; on a timescale ofa few bar rotation periods.Comment: AAS Latex and Postcript Figures, accepted for publication in Ap

Discovery of a Boxy Peanut‐shaped Bulge in the Near‐Infrared